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, Second Edition . 
William H. Hayi, Jr. Jack E. Kemmerh 
International Student Edition 

f . W©oeLo»<A _ 

Engineering Circuit Analysis 



T«l. Rochdale 50514 


Frederick Emmons Terman, Consulting Editor 

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Engineering Circuit Analysis 

Second Edition 

William H. Hayt, Jr. 

Professor of Electrical Engineering 
Purdue University 

Jack E. Kemmerly 

Professor of Engineering 
California State College, Fullerfon 

International Student Edition 

McGraw-Hill Book Company 

New York 

St. Louis 

Son Francisco 







Kogakusha Company, Ltd. 


Engineering Circuit Analysis 


Exclusive rights by Kogakusha Co., Ltd., for manufacture and 
export from Japan. This book cannot be re-exported from the 
country to which it is consigned by Kogakusha Co., Ltd., or 
by McGraw-Hill Book Company or any of its subsidiaries. 


Copyright © 1962, 1971 by McGraw-Hill, Inc. All rights reserved. 
No Part of this publication may be reproduced, stored in a 
retrieval system, or transmitted, in any form or by any means, 
electronic, mechanical, photocopying, recording, or otherwise, 
without the prior written permission of the publisher. 

Library of Congress Catalog Card Number 70-141920 



2-7 Voltage and Current Division 


PART ONE: The Resistive Circuit 

Chapter One 

Definitions and Units 3 

1-1 Introduction o 

1 -2 Systems of Units . 

1 -3 The Unit of Charge a 

1-4 Current, Voltage, and Power jg 

1 -5 Types of Circuits and Circuit Elements j 7 

Chapter Two 

Experimental Laws and Simple Circuits 24 

2-1 Introduction 
2-2 Ohm's Law 


2-3 Kirchhoff's Laws ,7 

2-4 Analysis of a Single-loop Circuit 33 

2-5 The Single Node-pair Circuit 

2-6 Resistance and Source Combination jq 


Chapter Three 

Some Useful Techniques of Circuit Analysis 53 

3-1 Introduction 
3-2 Nodal Analysis 
'3-3 Mesh Analysis 
3-4 Source Transformations 
3-5 Linearity and Superposition 
3-6 Thevenin's and Norton's Theorems g 4 

3-7 Trees and General Nodal Analysis 
3-8 Links and Loop Analysis 



yjjj Contents 

PART TWO: The Transient Circuit 

Chapter Four 

Inductance and Capacitance 109 

4-1 Introduction 109 

4-2 The Inductor 110 

4-3 Integral Relationships for the Inductor 1 1 5 

4-4 The Capacitor 1 20 

4-5 Inductance and Capacitance Combinations 127 

4-6 Duality 132 

4-7 Linearity and Its Consequences Again 1 37 

Chapter Five 

Source-free RL and RC Circuits 142 

5-1 Introduction 142 

5-2 The Simple RL circuit 144 

5-3 Properties of the Exponential Response 1 48 

5-4 A More General RL Circuit 1 51 

5-5 The Simple RC Circuit 1 54 

5-6 A More General RC Circuit 1 58 

5-7 General RL and RC Circuits 159 

Chapter Six 

The Application of the Unit-step Forcing Function 1 70 

6-1 Introduction > 70 

6-2 The Unit-step Forcing Function 171 

6-3 A First Look at the Driven RL Circuit 176 

6-4 The Natural and the Forced Response 180 

6-5 RL Circuits 182 

6-6 RC Circuits 188 

Chapter Seven 

The RLC Circuit 195 

7- 1 Introduction 1 95 

7-2 The Source-free Parallel Circuit 197 

7-3 The Overclamped Parallel RLC Circuit 201 

7-4 Critical Damping 205 

7-5 The Underdamped Parallel RLC Circuit 210 

7-6 The Source-free Series RLC Circuit 215 

7-7 The Complete Response of the RLC Circuit 218 

PART THREE: Sinusoidal Analysis 

Chapter Eight 

The Sinusoidal Forcing Function 233 

8-1 Introduction 233 

8-2 Characteristics of Sinusoids 235 

8-3 Forced Response to Sinusoidal Forcing Functions 238 

IX Contents 

Chapter Nine 

The Phasor Concept 245 

9-1 Introduction 245 

9-2 The Complex Forcing Function 246 

P-3 The Phasor 251 

9-4 Phasor Relationships for R, L, and C 256 

9-5 Impedance 261 

9-6 Admittance 264 

Chapter Ten 

The Sinusoidal Steady-state Response 269 

10-1 Introduction 269 

10-2 Nodcl, Mesh, and Loop Analysis 270 

10-3 Superposition, Source Transformations, and Thevenin's Theorem 272 

10-4 Phasor Diagrams 275 

1 0-5 Response as a Function of w 280 

Chapter Eleven 

Average Power and RMS Values 289 

11-1 introduction 

1 1-2 Instantaneous Power 

1 1 -3 Average Power 293 

1 1-4 Effective Values of Current and Voltage 302 

1 1-5 Apparent Power and Power Factor 306 

11-6 Complex Power 3qo 

Chapter Twelve 

Polyphase Circuits 317 

12-1 Introduction 317 

12-2 Single-phase Three-wire Systems 32] 

1 2-3 Three-phase Y-Y Connection 325 

1 2-4 The Delta (A) Connection 33^ 

1 2-5 Use of the Wattmeter 335 

1 2-6 Power Measurement in Three-phase Systems 337 



PART FOUR: Complex Frequency 

Chapter Thirteen 

Complex Frequency 351 

13-1 Introduction 351 

1 3-2 Complex Frequency 353 

13-3 A Further Interpretation of Complex Frequency 356 

1 3-4 The Damped Sinusoidal Forcing Function 353 

1 3-5 Z(s) and Y(s} 362 

13-6 Frequency Response as a Function of a 366 

1 3-7 The Complex-frequency Plane 3/j 

13-8 Natural Response and the s Plane 382 

Chapter Fourteen 

Frequency Response 394 

14-1 Introduction 304 

14-2 Parallel Resonance 396 

X Contents 

1 4-3 Series Resonance 409 

14-4 Other Resonant Forms 411 

14-5 Scaling 417 

PART FIVE: Two-port Networks 

Chapter Fifteen 

Magnetically Coupled Circuits 431 

15-1 Introduction 431 

15-2 Mutual Inductance 432 

15-3 Energy Considerations 441 

15-4 The Linear Transformer 447 

1 5-5 The Ideal Transformer 453 

Chapter Sixteen 

Two-port Networks 468 

16-1 Introduction 468 

16-2 One-port Networks 469 

16-3 Admittance Parameters 473 

16-4 Some Equivalent Networks 479 

16-5 Impedance Parameters 485 

1 6-6 Hybrid Parameters 490 

PART SIX: Network Analysis 

Chapter Seventeen 

Fourier Analysis 503 

17-1 Introduction 503 

17-2 Trigonometric Form of the Fourier Series 506 

17-3 The Use of Symmetry 513 

17-4 Complete Response to Periodic Forcing Functions 518 

17-5 Complex Form of the Fourier Series 521 

Chapter Eighteen 

Fourier Transforms 531 

18-1 Introduction 531 

18-2 Definition of the Fourier Transform 532 

1 8-3 Some Properties of the Fourier Transform 537 

18-4 The Unit-impulse Function 541 

1 8-5 Fourier Transform Pairs for Some Simple Time Functions 546 

18-6 The Fourier Transform of a General Periodic Time Function 552 

18-7 Convolution and Circuit Response in the Time Domain 554 

18-8 The System Function and Response in the Frequency Domain 559 

18-9 The Physical Significance of the System Function 563 

Chapter Nineteen 

Laplace Transform Techniques 573 

19-1 Introduction 573 

1 9-2 Definition of the Laplace Transform 575 

19-3 Laplace Transforms of Some Simple Time Functions 578 

19-4 Several Basic Theorems for the Laplace Transform 581 

1 9-5 Convolution Again 588 

19-6 Time-shift and Periodic Functions 591 

XJ Content* 

19-7 Shifting, Differentiation, Integration, and Scaling in the Frequency Domain 596 

19-8 The Initial-value and Final-value Theorems 600 

1 9-9 The Transfer Function H(s) 602 

19-10 The Complete Response 605 

PART SEVEN: Appendixes 

Appendix One 

Determinants 619 

Appendix Two 

A Proof of Thevenin's Theorem 624 

Appendix Three 

Complex Numbers 628 

Index M3 


This book is intended for use with a first course in electrical engineering. 
In many colleges and universities such a course will be preceded or accom- 
panied by an introductory physics course in which the basic concepts of 
electricity and magnetism are introduced, most often from the field 
aspect. Such a background is not a prerequisite, however. Instead, sev- 
eral of the requisite basic concepts of electricity and magnetism are dis- 
cussed (or reviewed) in the first chapter. Only a basic course in the dif- 
ferential and integral calculus need be considered as a prerequisite, or 
possibly a corequisite, to the reading of the book. Circuit elements are 
introduced and defined here in terms of their circuit equations; only inci- 
dental comments are offered about the pertinent field relationships. 

It is the authors' intention that this text be one from which a student 
may teach himself; it is written to the student and not to the instructor. 
If at all possible, each new term is clearly defined when it is first intro- 
duced. The basic material appears toward the beginning of each chapter 
and is explained carefully and in detail; numerical examples are usually 
used to introduce and suggest general results. Drill problems appear at 
the end of most sections; they are generally simple, and the answers to the 
three parts are given in random order. The more difficult problems which 
appear at the end of the chapters are in the general order of presentation 
of the text material. These problems are occasionally used to introduce 
less important or more advanced topics through a guided step-by-step 
procedure, as well as to introduce topics which will appear in the follow- 
ing chapter. The introduction and resulting repetition are both important 
to the learning process. In all, there are 234 drill problems, each consist- 
ing of three parts, and 447 additional problems at the ends of the chapters. 
These problems are all new in this edition. 

The general order of the material has been selected so that the student 
may learn as many of the techniques of circuit analysis as possible in the 
simplest context, namely, the resistive circuit which is the subject of the 



first part of this text. Basic laws, a few theorems, and some elementary 
network topology enable most of the basic analytical techniques to be 
developed. Numerous examples and problems are possible since the solu- 
tions are not mathematically complicated. The extension of these tech- 
niques to more advanced circuits in subsequent parts of the text affords 
the opportunity both for review and generalization. This first part of the 
text may be covered in three to six weeks, depending on the students' 
background and ability, and on the course intensity. 

The second part of the text is devoted to the natural response and the 
complete response to dc excitation of the simpler RL, RC, and RLC cir- 
cuits. Differential and integral calculus are necessary, but a background 
in differential equations is not required. The unit step is introduced as an 
important singularity function in this part, but the introduction of the 
unit impulse is withheld until the sixth part when our need for it is greater. 

The third part of the text introduces the frequency domain and initiates 
operations with complex numbers by concentrating on sinusoidal analysis 
in the steady state. Part three also includes a discussion of average power, 
rms values, and polyphase circuits, all of which are associated with the 
sinusoidal steady state. 

In the fourth part of the book the complex-frequency concept is intro- 
duced and its use in relating the forced response and the natural response 
is emphasized. The determination of the complete response of sinusoidally 
excited circuits begins to tie together the material of the first three parts. 

The fifth part begins with a consideration of magnetic coupling, which 
is basically a two-port phenomenon, and logically leads into a considera- 
tion of two-port network analysis and the linear modeling of various elec- 
tronic devices. 

Part six of the text describes the use of transform methods in circuit 
analysis. Starting with the Fourier series description of periodic wave- 
forms, the treatment is extended to nonperiodic forcing and response func- 
tions, using the Fourier transform. The final chapter covers the more 
important Laplace transform techniques and their use in obtaining the 
complete response of more complicated circuits. 

It is felt that the material in this book is more than adequate for a 
two-semester course, but some selection may be made from the last four 
or five chapters. No material is included in the text which will not be of 
some value in the following term; thus, signal-flow graphs, the relationship 
of circuit theory to field theory, advanced topological concepts, and the 
details of computer-aided analysis are among those subjects which are 
relegated to subsequent courses. The goal is the student's ability to write 
correct circuit equations for any circuit and his ability to solve the less 
complex cases and to understand the solutions. 

A number of changes have been made in this revision. The generally 
accepted International System of Units has been adopted in this edition, 

XV Preface 

and a notational summary is provided inside the back cover. The mate- 
rial on topology is presented earlier in the text, where it can be utilized to 
greater advantage. The problems, which have undergone the scrutiny of 
thousands of students and teachers, have all been replaced. The last two 
chapters on Fourier and Laplace transforms are new and provide more 
powerful analytical tools with which to attack problems that defy the 
more elementary approaches. Finally, the authors wished to place a 
greater emphasis on dependent voltage and current sources, thus permitting 
models for electronic devices to be studied from the outset. 

Throughout the book there is a logical trail leading from definition, 
through explanation, description, illustration, and numerical example, to 
problem-solving ability and to the obvious expectation of the authors 
that the student continually ask himself, "Why does this happen? How is 
it related to last week's work? Where do we logically go next? " There 
is a tremendous amount of enthusiastic momentum in a beginning engi- 
neering student, and this may be preserved by providing frequent drill 
problems whose successful solution confirms the student's progress in his 
own mind, by integrating the various sections into a coherent whole, by 
pointing out future applications and more advanced techniques, and by 
maintaining an interested, inquisitive attitude in the student. 

If the book occasionally appears to be informal, or even lighthearted, 
it is because the authors feel that it is not necessary to be dry or pompous 
to be educational. An amused smile on the face of a student is seldom an 
obstacle to his absorbing information. If the writing of the text had its 
entertaining moments, then why not the reading too? 

Much of the material in the text is based on courses taught at Cali- 
fornia State College, Fullerton, and at Purdue University. 

William H. Hayt, Jr. 
Jack E. Kemmehly 

Engineering Circuit Analysis 

Chapter One 
Definitions and Units 


'fyetBty yews ago, an introductory textbook on eleetric-eircuit analysis 
woidd have begun wi&a description of the electrical engineer's place to 
'science asd industry, ids glorious achievements of the past, and die lucrative \ 
and challenging Itfe ahead. Now, however, it is becoming increasingly 
conanon for students of mechanical engineering, civil engineering, chemical 
engineering, and other engineering curricula, as well as an occasional 
student -of mathematics or physics, to study introductory circuit analysis j 
with die efectricaj engineer. As a matter of fact, courses based largely oft' 
beginning circuit analysis are now being taken by engineering students 

4 Tke Resistive Circuit 

before they have become identified with a particular branch of engineering. 

If we have already entered or intend to enter an electrical engineering 
program, then circuit analysis simply may represent the introductory course 
in our chosen field. If we are associated with some other branch of engi- 
neering, then circuit analysis may represent a large fraction of our total 
study of electrical engineering, but it also enables us to continue our 
electrical work in electronics, instrumentation, and other areas. Most 
important, however, is the possibility given to us to broaden our educational 
base and become more informed members of a team which may be primar- 
ily concerned with the development of some electrical device or system. 
Effective communication within such a team can be achieved only if the 
language and definitions used are familiar to all. 

Few of the engineering accomplishments of the recent past can be 
credited to a single individual. The era of the Edison-type inventor has 
passed, and a graduating engineer should expect to become part of a group 
consisting of many kinds of engineers, applied mathematicians, and physi- 
cists. The group effort will be coordinated by technically trained managers, 
and the technical products will be produced, sold, and often operated and 
maintained by men having scientific or engineering training. The engi- 
neering graduates of today are not all employed solely to work on the 
technical design aspects of engineering problems. 

In order to contribute to the solution of these engineering problems, 
an engineer must acquire many skills, one of which is a knowledge of 
electric-circuit analysis. 

We shall begin this study by considering systems of units and several 
basic definitions and conventions. For those who have no knowledge of basic 
electricity and magnetism, the elementary subject material is included in 
this chapter. It should be rapid reading for anyone having an adequate 
background in introductory physics, but it should be read carefully by all. 
After these introductory topics have been mastered we can then turn our 
attention to a simple electric circuit. 


We must first establish a common language. Engineers cannot communicate 
with one another in a meaningful way unless each term used is clear and 
definite. It is also true that little learning can be achieved from a textbook 
which does not define carefully each new quantity as it is introduced. If 
we speak in the vague generalities of a television commercial — "gets clothes 
up to 40 per cent whiter" — and do not bother to define whiteness or to 
provide units by which it may be measured, then we shall certainly not 
succeed in engineering, although we might sell a lot of soap. 

In order to state the value of some measurable quantity, we must give 

5 Definition* and Units 

both a number and a unit, such as "3 inches." Fortunately we all use the 
same number system and know it well. This is not as true for the units, 
and some time must be spent in becoming familiar with a suitable system 
of units. We must agree on a standard unit and be assured of its permanence 
and its general acceptability. The standard unit of length should not be 
defined in terms of the distance between two marks on a certain rubber 
band; this is not permanent, and furthermore everybody else is using 
another standard. 

We shall also need to define each technical term at the time it is 
introduced stating the definition in terms of previously defined units and 
quantities. Here the definition cannot always be as general as the more 
theoretically minded might wish. For instance, it will soon be necessary 
to define "voltage." We must either accept a very complete and general 
definition, which we can neither appreciate nor understand now, or else 
adopt a less general but simpler definition which will satisfy our purposes 
for the present. By the time a more general definition is needed, our 
familiarity with the simpler concepts will help our understanding at that 

It will also become evident that many quantities are so closely related 
to each other that the first one defined needs a few subsequent definitions 
before it can be thoroughly understood. As an example, when the "circuit 
element" is defined it is most convenient to define it in terms of current 
and voltage, and when current and voltage are defined, it is helpful to do 
so with reference to a circuit element. None of these three definitions can 
be well understood until all have been stated. Therefore, our first definition 
of the circuit element may be somewhat inadequate, but then we shall 
define current and voltage in terms of a circuit element and finally, go 
back and define a circuit element more carefully. A later study of electro- 
magnetic theory should provide us with a more general definition of both 
current and voltage. 

We have very little choice open to us with regard to a system of units. 
The one we shall use was adopted by the National Bureau of Standards 
in 1964; it is used by all the major professional engineering societies and 
is the language in which today's textbooks are written. This is the Interna- 
tional System of Units (abbreviated SI in all languages), adopted by the 
General Conference on Weights and Measures in 1960. The SI is built upon 
six basic units: the meter, kilogram, second ampere, degree Kelvin, and 
candela. We shall look at the definitions of the first four of these basic 
units below. Standard abbreviations for them and other SI units are listed 
inside the back cover of this text and will be used throughout our discus- 

In the late 1700s the meter was defined to be exactly one ten-millionth 
of the distance from the earth's pole to its equator. This distance was 
marked off by two fine lines on a platinum-iridium bar which had been 

£ The Resistive Circuit 

cooled to zero degrees Celsius (°C) (formerly centigrade). Although more 
accurate surveys have shown since that the marks on the bar do not 
represent this fraction of the earth's meridian exactly, the distance between 
the marks was nonetheless accepted internationally as the definition of the 
standard meter until 1960. In that year the General Conference agreed 
to define the meter (m) as 1,650,763.73 times the wavelength of radiation 
of the orange line of krypton 86. The definitions are equivalent, but the 
newer definition is more permanent and reproducible. 

The basic unit of mass, the kilogram (kg), was defined in 1901 as the 
mass of a platinum block kept with the standard meter bar at the Interna- 
tional Bureau of Weights and Measures in Sevres, France. This definition 
was reaffirmed in 1960. The mass of this block is approximately equal to 
1000 times the mass of 1 cm 3 of pure water at 4°C. 

The third basic unit, the second (s), was defined prior to 1956 as 
%e,40o or a mean solar day. At that time it was defined as % x 556 925 9747 
of the tropical year 1900. In 1964 it was defined more carefully as 
9,192,631,770 periods of the transition frequency between the hyperfine 
levels F = 4, m F - and F = 3, m F = of the ground state 2 S 1/2 of 
the atom of cesium 133, unperturbed by external fields. This latter defini- 
tion is permanent and more reproducible than the former; it is also com- 
prehensible only to atomic physicists. However, any of these definitions 
adequately describes the second with which we are all familiar. 

The definition of the fourth basic unit, the ampere (A), will appear later 
in this chapter after we are more familiar with the basic properties of 
electricity. The remaining two basic units, the degree Kelvin (°K) and the 
candela (cd), are not of immediate concern to circuit analysts. 1 

The SI incorporates the decimal system to relate larger and smaller 
units to the basic unit and uses standard prefixes to signify the various 
powers of ten. These are: 

atto- (a-, 10- 18 ) deci- (d-, 10" *) 



IO" 15 ) 



-, 10 1 ) 


(p- ; 

, io- 12 ) 



IO 2 ) 



10" 9 ) 



IO 3 ) 



io- 6 ) 



, 10 s ) 



, io- 3 ) 



, IO 9 ) 



IO" 2 ) 



IO 12 ) 

'Complete definitions of all the basic units and a further discussion of the International System 
of Units may be found in R. D. Huntoon, Status of National Standards for Physical Measure- 
ments, Science, vol. 150, no. 3693, pp. 169-178, Oct. 8, 1965, or in C. H. Page et al., IEEE 
Recommended Practice for Units in Published Scientific and Technical Work, IEEE Spectrum, 
vol. 3, no. 3, pp. 169-173, March, 1966. 

7 Definitions and Units 

These prefixes are worth memorizing, for they will appear often, both 
in this text and in other scientific work. Thus, a millisecond (ras) is y i000 
of a second, and a kilometer (km) is 1000 m. It is apparent now that the 
gram (g) was originally established as the basic unit of mass, and the 
kilogram then represented merely 1000 g. Now the kilogram is our basic 
unit, and we could describe the gram as a millikilogram if we wished to 
be confusing. Combinations of several prefixes, such as the millimicro- 
second, are unacceptable; the term nanosecond should be used. Also 
officially frowned on is the use of micron for 10~ 6 m; the correct term 
is the micrometer (jim). The angstrom (A), however, may be used for 
10- 10 m. 

This power-of-10 relationship is not present in the so-called British 
System of Units, which is in common use in this country. There are many 
occasions when the results of an engineering analysis must be transformed 
into the British System of Units for use in the shop or for clarity in discus- 
sions with others. 

Most of us have a better mental picture of 2 in. than we do of 5 cm, 
although this great dependence on the older system is gradually changing. 

The fundamental British units are defined in terms of the SI units as 
follows: 1 in. is exactly 0.0254 m, 1 pound-mass (lbm) is exactly 
0.453 592 37 kg, and the second is common to both systems. 

As a last item in our discussion of units, we consider the three derived 
units used to measure force, work or energy, and power. The newton (N) 
is the fundamental unit of force, 2 and it is the force required to accelerate 
a 1-kg mass by one meter per second per second (1 m/s 2 ). A force of 1 N 
is equivalent to 0.22481 pound of force (lbf), and the average nineteen- 
year-old male, having a mass of 68 kg, exerts a force of 670 N on the 

The fundamental unit of work or energy is the joule (J), defined as one 
newton-meter (N-m). The application of a constant 1-N force through a 
1-m distance requires an energy expenditure of 1 J. The same amount of 
energy is required to lift this book, weighing about 10 N, a distance of 
approximately 10 cm. The joule is equivalent to 0.73756 foot pound-force 

The last derived quantity with which we shall concern ourselves is 
power, the rate at which work is done or energy is expended. The funda- 
mental unit of power is the watt (W), defined as 1 J/s. One watt is 
equivalent to 0.73756 ft-lbf/s. It is also equivalent to y 745 7 horsepower 
(hp), a unit which is now being phased out of engineering terminology. 

NOTE: Throughout the text, drill problems appear following sections in which 
a new principle is introduced, in order to allow the student to test his under- 

2 It is worth noting that all units named after famous scientists have abbreviations beginning 
with capital letters. 

3 The Resistive Circuit 

standing of the basic fact itself. The problems are useful in gaining familiarization 
with new terms and ideas and should all be worked. More general problems 
appear at the ends of the chapters. The answers to the drill problems are given 
in random order. For example, in Drill Prob. 1-1, the answers are (a) 1.09, (b) 2.00, 
and (c) 1.67. 

Drill Problems 

1-1 Fill in each of the following blanks: (a) 0.24 lbm = 
(b) 2 X 10 4 dm = km; (c) 10 5 ms = min. 


Ans. 1.09; 1.67; 2.00 

1 -2 Determine the average power required: (a) in watts, for a 150-lbf man to 
ascend a 10-ft ladder in 4 s; (b) in kilowatts, to accelerate a 2-ton-mass automobile 
from a standstill to 60 mi/h in 7 s; (c) in picowatts, to accelerate an electron 
(mass = 9.11 X 10~ 31 kg) from rest to 10 6 m/s in 1.5 ns. 

Ans. 93; 304; 508 


Before beginning a discussion of electricity and electric circuits, we may 
define in terms of an analogy the class of electrical phenomena which we 
are going to consider. When we hold a baseball out at arm's length and 
release it, we know that it falls toward the earth because of the gravitational 
force exerted on it. We can also describe precisely how it accelerates, what 
its velocity is at any given instant, when it reaches a given point, and where 
it will be at a given instant. Few of us understand, however, why it falls. 
Although we understand very well what gravitational forces do, we do not 
know what they are. 

In an analogous way, an electrical engineer is very familiar with the 
forces, meter deflections, heating effects, and other measurable responses 
caused by electricity, but he is only rarely concerned with the theoretical 
(and philosophical) nature of electricity itself. Therefore, our goal is a 
competence in observing electrical phenomena, describing them mathe- 
matically, and putting them to a practical use. We shall be only incidentally 
concerned with their cause. 

Suppose that we take a small piece of some light material such as pith 
and suspend it by a fine thread. If we now rub a hard rubber comb with 
a woolen cloth and then touch the pith ball with the comb, we find that 
the pith ball tends to swing away from it; a force of repulsion exists between 
the comb and the pith ball. After laying down the comb and then ap- 
proaching the pith ball with the woolen cloth, we can see that there is 

9 Definitions and Unit* 

a force of attraction present between the pith ball and the woolen cloth. 

We explain both of these forces on the pith ball by saying that they 
are electrical forces caused by the presence of electrical charges on the pith 
ball, the comb, and the woolen cloth. In an analogous way, we attribute 
the force on the baseball to a gravitational force caused by the presence 
of gravitational masses in the baseball and the earth. 

Our experiment shows clearly that the electrical force may be one of 
either attraction or repulsion, and in this respect the gravitational analogy 
breaks down. As far as we know at the present time, a gravitational 
repulsive force does not exist. 

We explain the existence of an electrical force of both attraction and 
repulsion by the hypothesis that there are two kinds of charge and that 
like charges repel and unlike charges attract. The two kinds of charge are 
called positive and negative, although we might have called them gold and 
black or vitreous and resinous (as they were termed many years ago). 
Arbitrarily, the type of charge originally present on the comb was called 
negative by Benjamin Franklin, and that on the woolen cloth, positive. 

We may now describe our experiment in these new terms. By rubbing 
the comb with the cloth, a negative charge is produced on the comb and 
a positive charge on the cloth. Touching the pith ball with the comb 
transferred some of its negative charge to the pith ball, and the force of 
repulsion between the like kinds of charge on the pith ball and comb caused 
the ball to move away. As we brought the positively charged woolen cloth 
near the negatively charged pith ball, a force of attraction between the 
two different kinds of charge was evident. 

We also know now that all matter is made up of fundamental building 
blocks called atoms and that the atoms, in turn, are composed of different 
kinds of fundamental particles. The three most important particles are the 
electron, the proton, and the neutron. The electron possesses a negative 
charge, the proton possesses an equal-magnitude positive charge, and the 
neutron is neutral, or has no charge at all. As we rubbed the rubber comb 
with the woolen cloth, the comb acquired its negative charge because some 
of the electrons on the wool were rubbed off onto the comb; the cloth 
then had an insufficient number of electrons to maintain its electrical 
neutrality and thus behaved as a positive charge. 

The mass of each of the three particles named above has been deter- 
mined experimentally and is 9.10908 X 10~ 31 kg for the electron and about 
1840 times as large for the proton and the neutron. 

Now we are ready to define the fundamental unit of charge, called the 
coulomb after Charles Coulomb, the first man to make careful quantitative 
measurements of the force between two charges. The coulomb can, of 
course, be defined in any way we wish as long as the definition is convenient, 
universally accepted, permanent, and does not contradict any previous 
definition. Again, this leaves us no freedom at all because the definition 

1 The Resistive Circuit 

which is already universally accepted is as follows: two small, identically 
charged particles which are separated one meter in a vacuum and repel 
each other with a force of 10~ 7 c 2 newtons possess an identical charge of 
either plus or minus one coulomb (C). The symbol c represents the velocity 
of light, 2.997925 X 10 8 m/s. In terms of this unit, the charge of an 
electron is a negative 1.60210 X 10" 19 C, and 1 C (negative) therefore 
represents the combined charge of about 6.24 X 10 18 electrons. 

We shall symbolize charge by O or q; the capital letter is reserved for 
a charge which does not change with time, or is a constant, and the 
lowercase letter represents the general case of a time-varying charge. We 
often call this the instantaneous value of the charge and may emphasize 
its time dependence by writing it as q(t). This same use of capital and 
lowercase letters will be carried over to all other electrical quantities as 

Drill Problem 

1 -3 Find the charge in aC represented by: (a) 7 electrons; (b) 15 protons; (c) the 
combination of 15 protons and 7 electrons. 

Ans. -1.12; 1.28; 2.40 aC 


The electrical phenomena discussed above belong to the field of elec- 
trostatics, which is concerned with the behavior of electric charges at rest. 
This is of interest to us only because it is a beginning and serves as a useful 
device to define charge. 

One part of the experiment, however, departed from electrostatics, the 
process of transferring charge from the wool cloth to the comb or from 
the comb to the pith ball. This idea of "transfer of charge" or "charge 
in motion" is of vital importance to us in studying electric circuits, because, 
in moving a charge from place to place, we may also transfer energy from 
one point to another. The familiar cross-country power transmission line 
is a practical example. 

Of equal importance is the possibility of varying the rate at which the 
charge is transferred in order to communicate or transfer intelligence. This 
process is the basis of communication systems such as radio, television, and 

Charge in motion represents a current, which we shall define more 
carefully below. The current present in a discrete path, such as a metallic 
wire, has both a magnitude and a direction associated with it; it is a measure 

] ] Definitions and Units 

of the rate at which charge is moving past a given reference point in a 
specified direction. We now consider a rather arbitrary example which, 
however, will lead us to the general definition of current as the time rate 
of change of charge, dq/dt. 

Let us consider a discrete path along which charge can move and ask 
a number of questions about the manner in which charge is traveling along 
this lead or conductor. As a first-hand observer, we shall place a very small 
student at point A on the path and ask him to record the total amount 
of charge which has passed him since some reference time t = 0. We ask 
that he take data every second 3 and then give him these detailed instruc- 

1 The positive direction is to your right. 

2 If positive charge moves past you in the positive direction, add the 
magnitude of the charge. 

3 If positive charge moves in the negative direction, subtract the 
charge magnitude. 

4 If negative charge moves in the positive direction, also subtract the 
charge magnitude. 

5 If negative charge moves in the negative direction, add the charge 

The observer watches for 8 s, records his data, and then hands us the 
graph, Fig. 1-1, explaining that q is the total charge which has moved past 
him since t — 0. 

3 He is a small, quick student. 

Fig. 1-1 A graph of the total charge q that has passed a given reference 
point since t = 0. The charge is measured over 1-s intervals. 


2 - 

->t (s) 

-1 ■ 

-2 - 

> t (s) 

Fig. 1-2 A graph of the instantaneous value of the total charge q{t) which 
has passed a given reference point since t = 0. 











6 7 



> « (s) 

Fig. 1-3 The instantaneous current, i = dq/dt y where q is given in Fig. 1-2. 

Now we see that there are many ways in which this record might be 
interpreted. For instance, in the first second either one unit positive charge 
moved by to the left or one negative charge moved past to the right. The 
same alternative is present for the second 1-s interval. As a matter of fact, 
in either of these intervals the observer might have had to count 100 unit 
positive charges moving to the right and 101 moving to the left. Perhaps 
positive and negative charges were in motion in both directions. 

It is fortunate that we do not need to know which specific one of this 
infinite number of possibilities actually occurred; the electrical effects 
produced by each will be the same. 

We now refine the data by making measurements much more often, 
and this requires that smaller and smaller elements of charge be counted. 
The limit is the amount of charge carried by a single electron. The 
graphical record now appears as a smooth curve, Fig. 1-2. 

We are now ready to consider the rate at which charge is being trans- 
ferred. In the time interval extending from t to (t + At), the charge 
transferred past the reference point has increased from q to (q + Aq). If 
the graph is decreasing at this instant, then Aq is a negative value. The 
rate at which charge is passing the reference point at time t is therefore 
very closely equal to Aq/At, and as the interval At decreases, the exact 
value of the rate is given by the derivative 


1 3 Definitions and Units 

at A(-.o A( 

We define the current at a specific point and flowing in a specified 
direction as the instantaneous rate at which net positive charge is moving 
past that point in the specified direction. Current is symbolized by J or i, 
and thus 


The unit of current is the ampere (A), which corresponds to charge moving 
at the rate of 1 C/s. The ampere was named after A. M. Ampere, a French 
physicist of the early nineteenth century. It is often called an "amp," but 
this is informal and unofficial. The use of the lowercase letter i is again 
to be associated with an instantaneous value. Using the data of Fig. 1-2, 
the instantaneous current is given by the slope of the curve at every point. 
This current is plotted in Fig. 1-3. 

The total charge transferred between time t and t may be expressed 
as a definite integral, 

= f i dt 

Several different types of current are illustrated in Fig. 1-4. A current 
which is constant is termed a direct current, or simply dc, and is shown 
by Fig. l-4a. We shall find many practical examples of currents which 
vary sinusoidally with time, Fig. l-4b; currents of this form are present 

Fig. 1-4 Several types of current: (a) Direct current, or dc. [b) Sinusoidal 
current, or ac. (c) Exponential current, (d) Damped sinusoidal current. 


I.^V 1 

> t 


<«) (b) 

Fig. 1 -5 Two methods of representation for the same current. 

in the normal household circuits. Such a current is often referred to as 
alternating current, or ac. Exponential currents and damped sinusoidal 
currents, sketched in Fig. l-4c and d, will also be encountered later. 

We establish a graphical symbol for current by placing an arrow next 
to the conductor. Thus, in Fig. l-5a the direction of the arrow and the 
value "3 A" indicate either that a net positive charge of 3 C/s is moving 
to the right or that a net negative charge of — 3 C/s is moving to the left 
each second. In Fig. l-5b there are again two possibilities: either —3 C/s 
is flowing to the left or +3 C/s is flowing to the right. All four of these 
statements and both figures represent currents which are equivalent in their 
electrical effects, and we say that they are equal. 

It is convenient to think of current as the motion of positive charge 
even though it is known that current flow in metallic conductors results 
from electron motion. In ionized gases, in electrolytic solutions, and in 
some semiconductor materials, positively charged elements in motion 
constitute part or all of the current. Thus, any definition of current can 
agree only with the physical nature of conduction part of the time. The 
definition and symbolism we have adopted are standard. 

We must next define a circuit element. Such electrical devices as fuses, 
light bulbs, resistors, batteries, capacitors, generators, and spark coils can 
be represented by combinations of simple circuit elements. We shall begin 
by showing a very general circuit element as a shapeless object possessing 
two terminals at which connections to other elements may be made, Fig. 
1-6. This simple picture may serve as the definition of a general circuit 
element. There are two paths by which current may enter or leave the 

Fig. 1-6 A general circuit element is characterized by a pair of terminals 
to which other general circuit elements may be connected. 


B o- 


1 5 Definition* and Units 

element. Later we shall define particular circuit elements by describing 
the electrical characteristics which may be observed at their pairs of 

Let us suppose that direct current is directed into terminal A of Fig. 
1-6, through the general element, and out of B. Let us also assume that 
the passage of this charge through the element requires an expenditure 
of energy. We then say that an electrical voltage or a potential difference 
exists between the two terminals, or that there is a voltage or potential 
difference "across" the element. Thus, the voltage across a terminal pah- 
is a measure of the work required to move charge through the element. 
Specifically, we shall define the voltage across the element as the work 
required to move a positive charge of 1 C from one terminal through the 
device to the other terminal. The sign of the voltage will be discussed 
below. The unit of voltage is the volt (V), which is i J/C and voltage is 
represented by V or v. We are indeed fortunate that the full name of the 
eighteenth-century Italian physicist, Alessandro Giuseppe Antonio Anastasio 
Volta, is not used for our unit of potential difference. 

The energy which is expended in forcing the charges through the 
element must appear somewhere else by the principle of conservation of 
energy. When we later meet specific circuit elements, we should note 
whether the energy is stored in some form which is readily available or 
whether it changes irreversibly into heat, acoustic energy, and so forth. 

We must now establish a convention by which we can distinguish 
between energy supplied to the element by some external source and energy 
which may be supplied by the element itself to some external device. We 
do this by our choice of a sign for the voltage of terminal A with respect 
to terminal B. If a positive current is entering terminal A of the element 
and if an external source must expend energy to establish this current, then 
terminal A is positive with respect to terminal B. Alternatively, we may 
say also that terminal B is negative with respect to terminal A. 

The sense of the voltage is indicated by a plus-minus pair of algebraic 
signs. In Fig. l-7a, for example, the placement of the plus sign at terminal 
A indicates that terminal A is v volts positive with respect to terminal B. 
If we later find that v happens to have a numerical value of —5 V, then 
we may say either that A is —5 V positive with respect to B or that B 

fig. 1-7 In (a) and (fo), terminal B is 5 V positive with respect to terminal 
A; in (c) and (d), terminal A is 5 V positive with respect to terminal B. 

] (f The Resistive Circuit 

is 5 V positive with respect to A. Other cases are shown and described 
in Fig. l-7b, c, and d. 

No statement can be made concerning energy transfer in any of these 
four cases until the direction of the current is specified. Let us assume 
that a current arrow is placed by each upper lead, directed to the right, 
and labeled " + 2 A"; then, since in both cases c and d terminal A is 5 V 
positive with respect to terminal B and since a positive current is entering 
terminal A, energy is being supplied to the element. In the remaining two 
cases, the element is delivering energy to some external device. 

We have already defined power, and we shall represent it by P or p. 
If one joule of energy is expended in transferring one coulomb of charge 
through the device, then the rate of energy expenditure in transferring one 
coulomb of charge per second through the device is one watt. The power 
must be proportional both to the number of coulombs transferred per 
second, or current, and to the energy needed to transfer one coulomb 
through the element, or voltage. Thus, 

p = vi 

Dimensionally, the right side of this equation is the product of joules per 
coulomb and coulombs per second, which produces the expected dimension 
of joules per second, or watts. 

With a current arrow placed by each upper lead of Fig. 1-7, directed 
to the right and labeled "2 A," 10 W is absorbed by the element in c and 
d and — 10 W is absorbed (or 10 W is generated) in a and b. 

The conventions for current, voltage, and power are summarized in 
Fig. 1-8. The sketch shows that if one terminal of the element is v volts 
positive with respect to the other terminal, and if a current i is entering 
the element through the first terminal, then a power p = vi is being 
absorbed by or delivered to the element. This convention should be studied 
carefully, understood, and memorized. In other words, it says that if the 
current arrow and the voltage polarity signs are placed at the terminals 
of the element such that the current enters that end of the element marked 
with the positive sign, and if both the arrow and the sign pair are labeled 

Rfl. 1 -8 The power absorbed by the element is given by the product, p =z vi. 

-3 A 

<•) (fc) (c) 

Fig. 1-9 (a) A power, p = (2p) = 6 W, is absorbed by the element. 
(6) A power, p = (-2)(-3) = 6 W, is absorbed by the element, (c) A 
power, p = (4)(-5) = -20 W, is absorbed by the element, or 20 W is 
delivered by the element. 

with the appropriate algebraic quantities, then the power absorbed by the 
element can be expressed by the algebraic product of these two quantities. 
If the numerical value of the product is negative, then the element is 
absorbing negative power or delivering power to some external element. 
The three examples of Fig. 1-9 further illustrate this convention. 

Drill Problems 

1 -4 The total charge q(t) entering the upper terminal of the circuit element 

in Fig. 1-8 is given by 20 e" - 2 ' sin (irt/4) C. Find i at t = : (a) 0; (b) 2 s; (c) -Is. 

Ans. -2.68; 15.7; 17.0 A 

1 -5 The current entering the upper terminal of the circuit element of Fig. 1-8 
is given by eOOt 2 - 8t A. If the total charge that has entered that terminal 
of the element is 60 /iC at t = - 10 ms, find q at t = : (a) -5 ms; (b) 0; (c) 10 ms. 

Ans. 460; 535; 660 jxC 

7-6 (a) If the power absorbed by the element of Fig. l-7fc is 30 W, find the 
current entering terminal B. (b) If the power absorbed by the element of Fig. 
l-7a is 30 W, find the current entering terminal A. (c) If the power delivered 
by the element of Fig. l-7d is 30 W, find the current entering terminal A. 

Ans. -6; -6; 6 A 


Using the concepts of current and voltage, it is now possible to be more 
specific in defining a circuit element. 

It is important to differentiate between the physical device itself and 
the mathematical model of this device which we shall use to analyze its 
behavior in a circuit. Let us agree that we will use the expression "circuit 

1 8 The Resistive Circuit 

element" to refer to the mathematical model. The choice of a particular 
model for any real device must be made on the basis of experimental data 
or experience; we shall usually assume that this choice has already been 
made. We must first learn the methods of analysis of idealized circuits. 

Now let us distinguish a general circuit element from a simple circuit 
element by the statement that a general circuit element may be composed 
of more than one simple circuit element, but that a simple circuit element 
cannot be further subdivided into other simple circuit elements. For 
brevity, we shall agree that the term circuit element generally refers to 
a simple circuit element. 

All the simple circuit elements that will be considered in the work that 
follows can be classified according to the relationship of the current through 
the element to the voltage across the element. For instance, if the voltage 
across the element is directly proportional to the current through it, or 
v = ki, we shall call the element a resistor. Other types of simple circuit 
elements have a terminal voltage which is proportional to the time deriva- 
tive or the integral with respect to time of the current. There are also 
elements in which the voltage is completely independent of the current 
or the current is completely independent of the voltage; these are the 
independent sources. Furthermore, we shall need to define special kinds 
of sources in which the source voltage or current depends upon a current 
or voltage elsewhere in the circuit; such sources will be termed dependent 
sources or controlled sources. 

By definition, a simple circuit element is the mathematical model of 
a two-terminal electrical device, and it can be completely characterized 
by its voltage-current relationship but cannot be subdivided into other 
two-terminal devices. 

The first element which we shall need is an independent voltage source. 
It is characterized by a terminal voltage which is completely independent 
of the current through it. Thus, if we are given an independent voltage 
source and are notified that the terminal voltage is 50f 2 V, we can be sure 
that at t = 1 s the voltage will be 50 V, regardless of the current that was 
flowing, is flowing, or is going to flow. The representation of an inde- 
pendent voltage source is shown in Fig. 1-10. The subscript s merely 
identifies the voltage as a "source" voltage. 

A point worth repeating here is that the presence of the plus sign at 

Fig. 1-10 The circuit symbol of an independent voltage source. The circuit 
symbol of a dependent or controlled voltage source is shown in Fig. 1-1 3a. 


] 9 Definition* and Units 

the upper end of the symbol for the independent voltage source in Fig. 
1-10 does not necessarily mean that the upper terminal is always positive 
with respect to the lower terminal. Instead, it means that the upper 
terminal is c 8 volts positive with respect to the lower. If, at some instant, 
v 8 happens to be negative, then the upper terminal is actually negative 
with respect to the lower at that instant. 

If a current arrow is placed adjacent to the upper conductor of this 
source and directed to the left, then the current i is entering the terminal 
at which the positive sign is located and the source thus absorbs a power 
p = vj. More often than not, a source is expected to deliver power to 
a network and not to absorb it. Consequently, we might choose to direct 
the arrow to the right in order that v s i will represent the power delivered 
by the source. Either direction may be used. 

The independent voltage source is an ideal source and does not represent 
exactly any real physical device, because the ideal source could theoret- 
ically deliver an infinite amount of energy from its terminals. Each coulomb 
passing through it receives an energy of t>, joules, and the number of 
coulombs per second is unlimited. This idealized voltage source does, 
however, furnish a reasonable approximation to several practical voltage 
sources. An automobile storage battery, for example, has a terminal voltage 
of 12 V that remains essentially constant as long as the current through 
it does not exceed a few amperes. The small current may have direction 
either through the battery, corresponding to power furnished by the 
battery to the headlights while it is discharging, or to power absorbed by 
the battery from the generator or a battery charger while it is charging. 
An ordinary household electrical outlet also approximates an independent 
voltage source provided the voltage v s = 115\/2 cos2w60f V; the repre- 
sentation is valid for currents less than perhaps 20 A. 

An independent voltage source which has a constant terminal voltage 
is often termed an independent dc voltage source and is represented by 
either symbol shown in Fig. 1-11. Note in Fig. 1-llfo that, when the 
physical plate structure of the battery is suggested, the longer plate is placed 
at the positive terminal; the plus and minus signs then represent redundant 
notation, but they are usually included anyway. 

Fig. 1-11 Alternative representations of a constant, or dc, independent 
voltage source. In (a) the source is delivering 12 W and in (fc) the battery 
is absorbing 1 2 W. 

6 V( 

8 V-S- 

(«) (4) 


Fig. 1-12 The circuit symbol of on independent current source. 

Another ideal source which we will need is the independent current 
source. Here, the current through the element is completely independent 
of the voltage across it. The symbol for an independent current source 
is shown in Fig. 1-12. If i, is constant, we call the source an independent 
dc source. 

Like the independent voltage source, the independent current source 
is at best a reasonable approximation for a physical element. In theory 
it can deliver infinite power from its terminals, because it produces the 
same finite current for any voltage across it, no matter how large that 
voltage may be. It is, however, a good approximation for many practical 
sources. For example, the independent dc source represents very closely 
the electron beam of a synchrotron which is operating at a constant beam 
current of perhaps 1 /iA and will continue to deliver 1 /iA to almost any 
device placed across its "terminals" (the beam and the earth). 

The two types of ideal sources that we have discussed up to now are 
called independent sources because the value of the source quantity is not 
affected in any way by activities in the remainder of the circuit. This is 
in contrast with yet another kind of ideal source, the dependent or controlled 
source, in which the source quantity is determined by a voltage or current 
existing at some other location in the electrical system under examination. 
To distinguish between independent and dependent sources, we introduce 
the additional symbols shown in Fig. 1-13. Sources such as these will appear 
in the equivalent electrical models for many electronic devices, such as 
transistors, vacuum tubes, and integrated circuits. We shall see all of these 
in the following chapters. 

Dependent and independent voltage and current sources are active 
elements; they are capable of delivering power to some external device. 
For the present we shall think of a passive element as one which is capable 

Fig. 1-13 The diamond shape characterizes the circuit symbols for (a) the 
dependent voltage source and [b) the dependent current source. 

•■<> 4 

o ' 

(a) (6) 



Fig. l-M (a) An electrical network which is not a circuit, (b) A network 
which is a circuit. 

only of receiving power. However, we shall later see that several passive 
elements are able to store a finite amount of energy and then return it 
later to an external element, and since we shall still wish to call such an 
element passive, it will be necessary to improve upon our two definitions 

The interconnection of two or more simple circuit elements is called 
an electrical network. If the network contains at least one closed path, 
we shall call it an electric circuit. Every circuit is a network, but not all 
networks are circuits. Figure l-14a shows a network which is not a circuit, 
and Fig. l-14fo shows a network which is a circuit. 

A network which contains at least one active element, such as an inde- 
pendent voltage or current source, is an active network. A network which 
does not contain any active elements is a passive network. 

Drill Problem 

1-7 Determine the power being supplied by the sources shown in Fig. l-15a, 
b, and c. 

Am. —21; -20; 18 W 




5V (J,)4A 

6 V 


(a) (6) 

Fig. 1-15 See Drill Prob. 1-7. 

-3 A 


6+ 7 V -i 



22 Th « R**i*Kv« Circuit 

□ 1 Curve (a) of Fig. 1-16 represents the total charge (q = y, in juC) that has passed 
a specified reference point in a given direction as a function of time (x = t, in 
ms). (a) How much charge passed the point between t = 3 and 6 ms? (b) What 
is the current at t = 4.2 ms? (c) What is the largest value of the current in the 
interval shown? 







2 4 6 8 

Fig. 1-16 Graphical relationships used in various problems. 


□ 2 Curve (b) of Fig. 1-16 represents the total charge (q = y, in nC) that has 
entered terminal A of a circuit element as a function of time (x = t, in jus), (a) 
How long a time is required for 2 nC to enter terminal A? (b) What is the value 
of the current entering terminal A at t = 2 jis? (c) Make a sketch of the current 
as a function of time, < t < 10 /is. 

D 3 Curve (a) of Fig. 1-16 represents the current (i = y, in A) at a certain point 
in a specified direction as a function of time (x = f, in ms). (a) How much charge 
passed the point between i = and 3 ms? (b) Between * = 3 and 6 ms? (c) At 
what rate is charge passing the point at t = 4 ms? 

□ 4 Curve (b) of Fig. 1-16 represents the current (i = y, in mA) entering terminal 
B of a circuit element as a function of time (x = f, in pis), (a) How much charge 
enters terminal B in the interval, 6 < t < 10 jus? (b) How long a time is required 
for 2 nC to enter terminal B? (c) Make a sketch of the charge that has entered 
terminal B as a function of time, < ( < 10 jus. 

D5 (a) If q — — 10 -7 e -105 ' C, find the average current during the time interval 
from t = — 5 fis to +5 fis. Given i = 12 cos (lOOOt + w/6) A; (b) find the average 
current during the interval, < t < w/3 ms; (c) determine the total charge 
transferred between t = and r = 2w/3 ms. 

23 Definition* and Unite 

□ 6 The charge (in C) that has entered a circuit element since t = — oo is numeri- 
cally equal to 50 times the current (in A) at that point for every instant of time. 

(a) If the current is 4 A at t = 10 s, find q(t). (b) If the total charge is 5 C at 
t = -20 s, find i(t). 

□ 7 A 12-V storage battery is charged by supplying a current entering its positive 
terminal that is a constant 3 A for 2 h and then decreases linearly to zero during 
the next hour. Assuming the battery voltage is constant: (a) What is the total 
charge delivered to the battery? (b) At what time is the power being delivered 
to the battery 24 W? (c) What is the average power delivered to the battery over 
the 3-h interval? (d ) How much energy is supplied to the battery? 

□ 8 For the independent current source shown in Fig. 1-12, t s = 10 sin lOOOf mA. 
Let the voltage of the upper terminal with respect to the lower be v. (a) If 
v = 25 sin 1000* V, find the power being absorbed by the source at t = 1.5w ms. 

(b) If v = 25 cos lOOOt V, find the power absorbed at r = 0.25V and 0.75w ms. 

□ 9 The output of a certain independent current source is a function of tempera- 
ture T(°K), i, = 10- 6 r 2 - 6 X 10r*T + 0.1 A. (a) At what temperature in the 
range 250 < T < 320°Kist J> a maximum? (b) At a constant temperature of 320 °K, 
how much charge can the source deliver at a voltage of 3722 V in 10 min? 

□ 1 Let the current i t enter the plus-marked terminal of a circuit element across 
which the voltage % is present. Find the power being absorbed by the element 
at t = 10 s if <! = 2 e- - 1 ' A and: (a) v t = 6 dijdt; (b) Cl = (y^Jfo dt + 2 V. 

Dll An independent current source t, and an independent voltage source c, are 
joined together by connecting the terminal with the arrowhead to the plus-marked 
terminal and then connecting the remaining two terminals together. The current 
leaving the current source is thus constrained to enter the voltage source. If 
v s = 2 cos 10 6 wf V and j 8 = 0.03 A, find the power absorbed by each source at: 
(a) t = 0;(b)t=l lis. 

D 12 The charge leaving the positive reference terminal of a voltage source is 
q = 6 sin 120w* - 8 cos 120rrt mC. If v, = 160 cos 120wr V: (a) find the power 
being supplied by the voltage source at t = 0; (b) find the average power supplied 
over the interval, < t < 1/60 s; (c) find the energy supplied by the source over 
the same time interval. 

25 Experimental Laws and Simple Circuits 

process by which the voltage and current associated with each element 
in a given circuit are determined. Fortunately, a complete analysis is not 
usually necessary, for often only a specific current, voltage, or perhaps 
power is needed. 

After a proficiency in analysis has been achieved in this and other early 
courses, problems in synthesis may be considered. Here we are given a 
mathematical description of the desired behavior of a circuit and must 
determine the necessary elements and their interconnection in order to 
obtain the desired response. Synthesis problems may often have more than 
one solution. 

The final type of circuit problem, and the one for which engineering 
salaries are most often paid, is that of design. A real, physical, manufac- 
turable, salable, economical, reliable device is the desired end product. 
Sometimes size, weight, temperature characteristics, and even eye appeal 
must be considered in the design. It is obvious that experience is a pre- 
requisite for design proficiency; it is also evident that analysis and synthesis 
must come first. 

This chapter and the following one are restricted to the analysis of 
simple circuits containing only current sources, voltage sources, and re- 
sistors; the sources may be independent or dependent. In analyzing these 
circuits we shall use several network transformations, network theorems, 
and mathematical methods which we shall later be able to apply, with only 
slight modifications, to circuits containing other types of passive elements 
excited by time-varying sources. We shall learn the methods useful in 
circuit analysis by applying them to the simplest possible case, the resistive 

2-2 OHM'S LAW 

The simplest passive element, the resistor, may be introduced by consider- 
ing the work of an obscure German physicist, George Simon Ohm, who 
published a pamphlet in 1827 entitled "Die galvanische Kette mathematisch 
bearbeitet." 1 In it were contained the results of one of the first efforts 
to measure currents and voltages and to describe and relate them mathe- 
matically. One result was a statement of the fundamental relationship we 
now call Ohm's law, even though it has since been shown that this result 
was discovered 46 years earlier in England by Henry Cavendish, a brilliant 
semirecluse. However, no one, including Ohm, we shall hope, knew of 
the work done by Cavendish because it was not uncovered and published 
until long after both were dead. 

Ohm's pamphlet received much undeserved criticism and ridicule for 

'"The Galvanic Circuit Investigated Mathematically." 

2 6 The R«i»tive Circuit 

several years after its first publication, but it was later accepted and served 
to remove the obscurity associated with his name. 

Ohm's law states that the voltage across many types of conducting 
materials is directly proportional to the current flowing through the mate- 

v - fit 

where the constant of proportionality K is called the resistance. The unit 
of resistance is the ohm, which is 1 V/A and customarily abbreviated by 
a capital omega, Q. 

When this equation is plotted on t> versus i axes, it is a straight line 
passing through the origin. The equation is a linear equation, and we shall 
consider it as the definition of a linear resistor. Hence, if the ratio of the 
current and voltage associated with any simple circuit element is a constant, 
then the element is a linear resistor and has a resistance equal to the 
voltage-current ratio. 

Again, it must be emphasized that the linear resistor is an idealized 
circuit element; it is a mathematical model of a physical device. "Resistors" 
may be easily purchased or manufactured, but it is soon found that the 
voltage-current ratio of this physical device is reasonably constant only 
within certain ranges of current, voltage, or power and depends also on 
temperature and other environmental factors. We shall usually refer to 
a linear resistor as simply a resistor, using the longer term only when the 
linear nature of the element needs emphasis. Any resistor which is nonlinear 
will always be described as such. Nonlinear resistors should not necessarily 
be considered as undesirable elements. Although it is true that their 
presence complicates an analysis, the performance of the device may 
depend on or be greatly improved by the nonlinearity. Zener diodes, tunnel 
diodes, and fuses are such elements. 

Figure 2-1 shows the most common circuit symbol used for a resistor. 
In accordance with the voltage, current, and power conventions adopted 
in the last chapter, the product of v and i gives the power absorbed by 
the resistor. This absorbed power appears physically as heat and is always 
positive; a resistor is a passive element that cannot deliver power or store 
energy. Alternative expressions for the absorbed power are 

p = vi = i 2 R = ^ 

Fig. 2-1 The circuit symbol for a resistor; R = v/i and p = vi = i 2 R = v 2 /R. 

»\ + « - 

o f S/S/ s s l o 


27 Experimental Laws and Simple Circuits 

The ratio of current to voltage is also a constant, 


where G is called the conductance. The unit of conductance is the mho, 
1 A/ V, and is abbreviated by an inverted omega, . The same circuit sym- 
bol is used to represent both resistance and conductance. The absorbed 
power is again necessarily positive and may be expressed in terms of the 
conductance by 

p = vi = v 2 G = i— 

Thus a 2-fl resistor has a conductance of % ®, and if a current of 5 A 
is flowing through it, a voltage of 10 V is present across the terminals and 
a power of 50 W is being absorbed. 

All the expressions above have been written in terms of instantaneous 
current, voltage, and power, such as v = Ri and p — vi. It is apparent 
that the current through and voltage across a resistor must both vary with 
time in the same manner. Thus, if R = 10 Q and t> = 2 sin lOOr V, then 
i — 0.2 sin lOOt A; the power, however, is 0.4 sin 2 lOOr W, and a simple 
sketch will illustrate the different nature of its variation with time. Al- 
though the current and voltage are each negative during certain time 
intervals, the absorbed power is never negative. 

Drill Problems 

2-1 With reference to Fig. 2-1, find v if: (a) G = 10" 2 !5 and i = -2.5 A; 

(b) R = 40 Q and the resistor absorbs 250 W; (c) i = 2.5 A and the resistor ab- 
sorbs 500 W. 

Ans. -250; ±100; 200 V 

2-2 If the current through a 10-kfi resistor is 2 cos 10 6 wt mA, and the voltage 
across it is positive at t = 0, find the voltage at t = : (a) 0.2 /is; (b) 0.5 fis; 

(c) 1 (IS. 

Ans. -20; 0; 16.2 V 


We are now ready to consider current and voltage relations in simple 
networks resulting from the interconnection of two or more simple circuit 
elements. The elements will be connected by electrical conductors, or 

Rfl. 2-2 [a) A circuit containing three nodes, [b) Node 1 is redrawn to look 
like two nodes; it is still one node. 

leads, which have zero resistance, or are perfectly conducting. Since the 
network then appears as a number of simple elements and a set of con- 
necting leads, it is called a lumped-constant network. A more difficult 
analysis problem arises when we are faced with a distributed-constant 
network, which essentially contains an infinite number of vanishingly small 
elements. This latter type of network is considered in later courses. 

A point at which two or more elements have a common connection 
is called a node. Figure 2-2a shows a circuit containing three nodes. 
Sometimes networks are drawn so as to trap an unwary student into 
believing that there are more nodes present than is actually the case. This 
occurs when a node, such as node 1 in Fig. 2-2a, is shown as two separate 
junctions connected by a (zero-resistance) conductor. However, all that 
has been done is to spread the common point out into a common line. 
Node 1 has been redrawn in this fashion in Fig. 2-2b. 

Another term whose use will prove convenient is a branch. We may 
define a branch as a single path containing one simple element which 
connects one node to any other node. The circuit shown in Fig. 2-2a and 
b contains five branches. 

We are now ready to consider the first of the two laws named for Gustav 
Robert Kirchhoff, a German university professor who was born about the 
time Ohm was doing his experimental work. This axiomatic law is called 
Kirchhoff s current law, and it states that the algebraic sum of all the 
currents entering any node is zero. 

Although we cannot rigorously prove the law at this time, 2 we should 
at least agree that it seems plausible. Suppose we consider the node shown 
in Fig. 2-3 at which three elements are joined together. Surrounding this 
node is a closed surface containing a volume V, within which we shall let 
the total charge be q. The total current entering V is therefore the algebraic 
sum of all the currents entering V, i A + i B + i c . This is equivalent to stating 

2 The proof is based on the hypothesis that charge is conserved, or that it can be neither 
created nor destroyed. We might just as well accept Kirchhoff's current law as being 
axiomatic instead of accepting the conservation of charge. 



Fig. 2-3 A closed surface surrounds a volume V and encloses a node; the 
total current entering the closed surface is zero: i A + i B + i c = 0. 

that charge is entering V at the rate of «! + *« + » c C/s. Hence, the charge 
q within V must be increasing at the rate of i A + i B + i c C/s, and 

'„+«* + «C = ^" 

Now we let V become vanishingly small and find that no electrical 
device other than the node itself is within V. A node, however, cannot 
store, destroy, or generate charge. Therefore, dq/dt must be zero, and 

'A + l B + 'C = ° 

This argument may be extended to any number of branches joined at a 

It is evident that we may also state Kirchhoff's current law in other 
ways. For instance, the algebraic sum of all the currents leaving a node 
is zero, or the algebraic sum of all the currents entering a node must equal 
the algebraic sum of all the currents leaving a node. These three forms 
lead directly to the three equivalent equations written below for the node 
shown in Fig. 2-4, 

i» + «b 

- «C - »D = ° 

»C + »D 

-i A -i B = 

l A + i B = V+ »D 

Fig. 2-4 Kirchhoff 's current law enables us to write i A + is — *c — *d = 0, 
'c + «o - 'a - *b = "/ or 'a + »B = 'c + *D- 


30 The Resistive Circuit 

A compact expression for Kirchhoff's current law is 


and this is just a shorthand statement for 

ij + « 2 + » 3 + • • • + i N = 

When this form is used, it is understood that the N current arrows either 
are all directed toward the node in question or are all directed away from 

It is sometimes helpful to interpret Kirchhoff's current law in terms 
of a hydraulic analogy. Water, like charge, cannot be stored at a point, 
and thus if we identify a junction of several pipes as a node, it is evident 
that the number of gallons of water entering the node every second must 
equal the number of gallons leaving the node each second. 

We now turn to Kirchhoff's voltage law. This law states that the 
algebraic sum of the voltages around any closed path in a circuit is zero. 
Again, we must accept this law as an axiom, even though it is developed 
in introductory electromagnetic theory. 

In view of our definition of the voltage across an element as the energy 
expended in moving a unit positive charge through the element, an equiva- 
lent statement of Kirchhoff's voltage law would seem to say that no energy 
is expended in moving the unit positive charge about any closed path. 
It turns out that this statement is correct for a circuit, or at least for its 
mathematical model; it is not true for a general path in a region of space 
containing time-varying magnetic fields. This statement may be clarified 
by considering a gravitational analogy. To raise a mass from a point at 
one elevation to a higher point and then to lower it to the original point 
requires no net expenditure of energy, regardless of the path taken. This 
interpretation corresponds to the application of Kirchhoff's voltage law 
to a circuit. However, let us suppose that there is a strong narrow jet of 
wind blowing upward at one point on the earth's surface. If we lift our 
mass outside the jet and then lower it within the jet, we must obviously 
do more work than if we had reversed the procedure, that is, raising it 
within the jet and lowering it outside. The work we do depends on the 
path. The presence of a time-varying magnetic field has much the same 
effect; the energy we expend in moving the charge depends on the particu- 
lar path we take through the magnetic field. Now, time-varying magnetic 
fields are intimately associated with inductors, as we shall see in Chap. 4, 
but Kirchhoff's voltage law may still be applied to circuits containing 
inductors. The reason is that, as soon as an inductance value is specified, 
a path is inferred. 

Kg. 2-5 A simple circuit used to emphasize the fact that Cj = v 2 

In summary, then, Kirchhoff's voltage law is applicable to circuits 
because physical devices are reduced to mathematical models in such a 
way that the law will be applicable. We should not be surprised to find 
that the work expended in carrying a unit positive charge around some 
more general closed path in space is not always zero. 

In a circuit, then, there is a single, definite value of energy associated 
with the two terminals of the element. Let us see how this statement leads 
to Kirchhoff's voltage law. Everybody who performs the coulomb-carrying 
experiment arrives at the same answer, regardless of the path taken in 
moving the charge about the circuit. Suppose that we have a choice of 
two paths along which we may move our charge from one point to another 
in a circuit, such as that available when two elements are connected as 
shown in Fig. 2-5. We may proceed from A to B either through the element 
on the left or through that on the right. We should expect the energy 
expended to be the same along either path. Thus the voltages t> 1 and v 2 
are equal, 

t>j = v 2 or v 2 — v 1 = 

Since v 2 — u t is the algebraic sum of the voltages around this closed path, 
then Kirchhoff's voltage law is satisfied. 

Let us consider this same circuit in a slightly different way by deter- 
mining the voltage between points B and C. We first carry our coulomb 
from B to A through the left element, supplying v t joules of electrical 
energy to our coulomb, and then proceed to C through the right element, 
losing t> 2 joules of electrical energy from our coulomb. The voltage between 
B and C along this path is thus 

~ v l + V 2 = V 2 - V t 

However, we might also choose the short path along the perfect conductor 

Fig. 2-6 Kirchhoff's voltage law leads to the equation — v l + v 2 — v 3 = 0. 

connecting B directly to C. The voltage here must be zero, for any nonzero 
voltage across a zero resistance will give rise to an infinite current which 
we reject as a physical impossibility. If we again assume that the voltage 
or energy obtained along different paths is the same, then, once more, 

e 2 - Oi = 

This latter point of view enables us to consider circuits composed of 
any number of elements connected in a single loop. Since the voltage across 
a short piece of one of the perfect conductors must be zero, then the voltage 
around the remainder of the circuit must be zero. Thus, we may write 


X C .= ° r v l + V 2 + V 3 + • • • + % = ° 


where we agree that every element is entered at its positive voltage 
reference in a clockwise (or counterclockwise) traversal of the circuit. 
We may apply Kirchhoff's voltage law in several different ways. For 
instance, in the circuit of Fig. 2-6, a clockwise trip around the circuit 
unfortunately meets one + sign and two (— ) signs. We might choose to 
reverse the signs across elements 1 and 3, letting those voltages be — v 1 
and — v 3 . It follows then that 

(-»l) +«2 + (-»3) =° 

We could instead reverse the voltage reference signs on element 2 and 
change the sign of « 2 ; counterclockwise travel then leads to 

«3 + (~ v 2) + V l = ° 

Usually, it is much easier to move around the circuit mentally, writing 
down directly the voltage of each element whose + terminal is entered 
and writing down the negative of every voltage first met at the minus sign. 


33 Experimental Laws and Simple Circuits 

Clockwise travel around the above circuit then gives 

— t)j + t> 2 — V 3 = 

whereas counterclockwise travel yields 

v 3 - V 2 + V l = ° 

These last four results are of course identical. 

Drill Problems 

2-3 Determine the number of branches and nodes present in each of the circuits 
of Fig. 2-7. 

Ans. 2, 2; 5, 4; 6, 4 

in SQ 

Fig. 2-7 See Drill Probs. 2-3, 2-4, and 2-5. 

2-4 Determine i x in each of the circuits of Fig. 2-7. 

2-5 Determine v x in each of the circuits of Fig. 2-7. 

Ans. -4; 1; 3 A 

Ans. -20; 15; 25 V 


Having established Ohm's and Kirchhoff 's laws, we may flex our analytical 
muscles by applying these tools in the analysis of a simple resistive circuit, 
such as the one shown in Fig. 2-8a. We shall assume that the resistance 
values and the source voltages are known and attempt to determine the 
current through each element, the voltage across each element, and the 
power delivered to or absorbed by each element. 

Our first step in the analysis is the assumption of reference directions 
for the unknown currents since we do not know a priori what these 

<o) (b) 

Fig. 2-8 [a) A single-loop circuit in which the source voltages and resistances 
are given, [b) Current and voltage reference signs have been added to the 

directions are. Arbitrarily, let us select an unknown current i which flows 
out of the upper terminal of the left voltage source. This choice is indicated 
by an arrow at that point in the circuit, as shown in Fig. 2-8fc. A trivial 
application of Kirchhoff 's current law assures us that this same current must 
also flow through every other element in the circuit. We may emphasize 
this fact this one time by placing several other current symbols about the 

By definition, all the elements that carry the same current are said to 
be connected in series. Note that elements may carry equal currents and 
not be in series; two 100-W lamp bulbs in neighboring houses may very 
well carry equal currents, but they do not carry the same current and are 
not in series. 

Our second step in the analysis is the choice of a voltage reference for 
each of the two resistors. We have already found that the application of 
Ohm's law, v = Ri, demands that the sense of the current and voltage be 
selected so that the current enters the terminal at which the positive voltage 
reference is located. If the choice of the current direction is arbitrary, then 
the selection of the voltage sense is fixed if we intend to use Ohm's law 
in the form v = Ri. The voltages v R1 and v R2 are shown in Fig. 2-8£>. 

The third step is the application of Kirchhoff's voltage law to the single 
closed path present. Let us decide to move around the circuit in the 
clockwise direction, beginning at the lower left corner, and write down 
directly every voltage first met at its positive reference and write down 
the negative of every voltage encountered at the negative terminal. Thus, 

~ V sl + V R1 + U s2 + V B2 = ° 

Finally, we apply Ohm's law to the resistive elements, 

%i = Ri* and v B2 = R 2 i 
and obtain 

-v sl + Rj + v s2 + R 2 i = 


Fig. 2-9 (a) A given series circuit, (fc) The circuit with current and voltage 
references assigned. 

This equation is solved for i, and thus 

R^ + R 2 

where all the quantities on the right side are known and enable us to 
determine i. The voltage or power associated with any element may now 
be obtained in one step by applying v = Ri, p — vi, or p = PR. 

Let us consider the numerical example illustrated in Fig. 2-9a. Two 
batteries and two resistors are connected in a series circuit. Currents and 
voltages are assigned to the circuit and indicated in Fig. 2-9£>, and Kirch- 
hoff's voltage law yields 

- 120 + v 30 + 30 + o 15 = 

An application of Ohm's law to each resistor permits us to write 

-120 + 30i + 30 + 15t = 

from which 

, 120 - 30 _ „ . 

' - 30 + 15 ~ 2 A 

Thus, the voltage across each resistor is 

u 30 = 2(30) = 60 V v 15 = 2(15) = 30 V 

The power absorbed by each element has been shown to be given by 
the product of the voltage across the element and the current flowing into 
the element terminal at which the positive voltage reference is located. 
For the 120-V battery, then, the power absorbed is 

p 120V = 120(-2) = -240 W 

and thus 240 W is delivered to other elements in the circuit by this source. 

36 Th * »«i»«v« Circuit 

In a similar manner, 

P30V = 30(2) = 60 W 

and we find that this nominally active element is actually absorbing power 
(or being charged), delivered to it by the other battery. 

The power absorbed by each resistor is necessarily positive and may 
be calculated by 

Pso = %>< = 60(2) = 120 W 
or by 

Pao = m = 2 2 (30) = 120 W 
and p 15 = v 15 i = i 2 R = 60 W 

The results check because the total power absorbed must be zero, or 
in other words, the power delivered by the 120-V battery is exactly equal 
to the sum of the powers absorbed by the three other elements. A power 
balance is often a useful method of checking for careless mistakes. 

Before leaving this example, it is important that we be convinced that 
our initial assumption of a direction for current flow had nothing to do 
with the answers obtained. Let us suppose that we assumed the current 
i to be directed in a counterclockwise direction. Both resistor voltages must 
then be assigned opposite directions also, and we should have obtained 

-120 -30t + 30 - 15t = 

and i = — 2 A, t> 30 = — 60 V, and « 15 = —30 V. Since each voltage 
reference is now reversed and each quantity is the negative of the previously 
obtained value, it is evident that the results are the same. Each absorbed 
power will be the same. 

Any random or convenient choice of current direction may be made. 
Those who insist on positive answers may always go back and reverse the 
direction of the current arrow and rework the problem. 

Now let us complicate the analysis slightly by letting one of the voltage 
sources be a dependent source, as exemplified by Fig. 2-10. We again assign 
a reference direction for the current i and the voltage t;^. There is no 
need to assign a voltage to the 15-0 resistor, since the controlling voltage 
v A for the dependent source is already available. It is worth noting, 
however, that the reference signs for v A are reversed from those we would 
have assigned, and that Ohm's law for this element must thus be expressed 
as v A = — 15i. We apply Kirchhoff 's voltage law around the loop, 

-120 + c 30 + 2o,-o 1 =0 

is n 

Fig. 2-10 A current i and voltage v^ are assigned in a single-loop circuit 
containing a dependent source. 

utilize Ohm's law twice, 

and obtain 

v A = -15i 

-120 + 30i - 30i + 15i = 
j = 8 A 

The power relationships show that the 120-V battery supplies 960 W, 
the dependent source supplies 1920 W, and the two resistors together 
dissipate 2880 W. 

More practical applications of the dependent source, such as transistor 
and vacuum-tube equivalent circuits, will begin to appear in the following 

Drill Problems 

2-6 For the circuit shown in Fig. 2-1 la, find the power: (a) delivered to the 
5-kfl resistor; (b) supplied by the — 25- V source; (c) supplied by the 10-V source. 

An*. -20; 20; 50 mW 

2-7 With reference to the circuit of Fig. 2-1 lb, find the power absorbed by: 
(a) the 100-fl resistor; (b) the 300-V source; (c) the dependent source. 

Ans. -1200; -640; 1600 W 

Fig. 2-1 1 See Drill Probs. 2-6 and 2-7. 
1 Va 5 ItQ 


1500 n 

-V s © 

0.4 c, 





- »x + 

— VvV- 

ioo a 



38 The Resistive Circuit 


The companion of the single-loop circuit discussed above is the single 
node-pair circuit in which any number of simple elements are connected 
between the same pair of nodes. An example of such a circuit is shown 
in Fig. 2-12a. The two current sources and the conductance values are 
known, and we are to find the voltage, current, and power associated with 
each element once more. 

Our first step is now to assume a voltage across any element, assigning 
an arbitrary reference polarity. Then Kirchhoff's voltage law forces us to 
recognize that the voltage across each branch is the same because a closed 
path proceeds through any branch from one node to the other and then 
is completed through any other branch. A total voltage of zero requires 
an identical voltage across every element. We shall say that elements 
having a common voltage across them are connected in parallel. Let us 
call this voltage v and arbitrarily select it as shown in Fig. 2-12b. 

Two currents, flowing in the resistors, are then selected in conformance 
with the convention established with Ohm's law. These currents are also 
shown in Fig. 2-12&. 

Our third step in the analysis of the single node-pair circuit is the 
application of Kirchhoff 's current law to either of the two nodes in the 
circuit. It is usually clearer to apply it to the node at which the positive 
voltage reference is located, and thus we shall equate the algebraic sum 
of the currents leaving the upper node to zero, 

- 120 + i 30 + 30 + i 15 = 

Finally, the current in each resistor is expressed in terms of v and the 
conductance of the resistor by Ohm's law, 

and we obtain 

i-m = 30t> and L. = 15u 

- 120 + 30o + 30 + 15t> = 

Fig. 2-12 (a) A single node-pair circuit, (fo) A voltage and two currents are 

39 Exparimantal lows and. Simpl* Circuih 


t> = 2 V 

*30 : 

The several values of absorbed power are now easily obtained. In the 
two resistors, 

Pan = 30(2) 2 = 120 W p 15 = 15(2) 2 = 60 W 

and for the two sources, 

p 120a = 120(-2) = -240 W P30a = 30(2) = 60 W 

Thus, the larger current source delivers 240 W to the other three 
elements in the circuit, and the conservation of energy is verified again. 

The similarity of this example to the one previously completed, illus- 
trating the solution of the series circuit with independent sources only, 
should not have gone unnoticed. The numbers are all the same, but currents 
and voltages, resistances and conductances, and "series" and "parallel" are 
interchanged. This is an example of duality, and the two circuits are said 
to be exact duals of each other. If the element values or source values 
were changed in either circuit, without changing the configuration of the 
network, the two circuits would be duals, although not exact duals. We 
shall study and use duality later, and at this time should only suspect that 
any result we obtain in terms of current, voltage, and resistance in a series 
circuit will have its counterpart in terms of voltage, current, and conduct- 
ance for a parallel circuit. 

With this introduction to the duality principle, let us consider the dual 
of Fig. 2-10, the series circuit containing a dependent source. The single 
node-pair circuit with a dependent current source is illustrated in Fig. 
2-13. A voltage v is assigned as shown, as is a current i^ through the 
30-0 conductance. Since the current in the 15-0 element is already denned 
as t^, we need assign no redundant current there. 

Fig. 2-13 A voltage v and current t^ are assigned in a single node-pair 
circuit containing a dependent source. 


40 Th * iMistiva Circuit 

Applying Kirchhoff's current law once, 

-i20 + i^ + 2i A - i A =0 
and Ohm's law twice, 

*30 = 30v 

-i A = 15t> 

we have 


- 120 + 30t) - 30t> + 15u = 
v = 8 V 

This corresponds to our previous result of 8 A, and duality triumphs again. 

Drill Problems 

2-8 In the circuit of Fig. 2-14a, find the energy absorbed in 1 h by the: (a) 1-mA 
source; (b) — 2-mA source; (c) 40-juU conductance. 

Arts. -108; 129.6; 216 J 

Fig. 2-14 See Drill Probs. 2-8 and 2-9. 

2-9 For the circuit of Fig. 2-146, find: (a) i i; (b) i 2 ; (c) t 3 . 

Ans. -6; -4; 2 A 


Some of the equation writing that we have been doing for the simple series 
and parallel circuits can be avoided. This is achieved by replacing relatively 
complicated resistor combinations by a single equivalent resistor whenever 


i. r 

Fig. 2-15 (a) A circuit containing a series combination of A? resistors, [b] A 
simpler equivalent circuit: /? eg = /?j + /{ 2 + • • • + B ff . 

we are not specifically interested in the current, voltage, or power associ- 
ated with any of the individual resistors in the combinations. All the 
current, voltage, and power relationships in the remainder of the circuit 
will be the same. 

We first consider the series combination of N resistors, shown sche- 
matically in Fig. 2-15a. The broken line surrounding the resistors is in- 
tended to suggest that they are enclosed in a "black box," or perhaps in 
another room, and we wish to replace the N resistors by a single resistor 
with resistance R eg so that the remainder of the circuit, in this case only 
the voltage source, does not realize that any change has been made. The 
source current, power, and, of course, the voltage will be the same before 
and after. 

We apply Kirchhoff 's voltage law 

v s = v 1 + v 2 + ■•■ + v N 

and Ohm's law 

c„ = fiji + R 2 i + ■■■ + R N i = (R 1 + R 2 + ■■■ + fl w )i 

and then compare this result with the simple equation applying to the 
equivalent circuit shown in Fig. 2-15fo, 

«, = «e«« 

Thus, the value of the equivalent resistance for N series resistances is 

R eQ = R 1 + R 2 + ■■■ +R N 

It should be emphasized again that we might be particularly interested 
in the current, voltage, or power of one of the original elements, as would 
be the case when the voltage of a dependent voltage source depends upon, 
say, the voltage across R 3 . Once R 3 is combined with several series resistors 
to form an equivalent resistance, then it is gone and the voltage across 


WN — HUHr 

10 n 30 v 7 a s o 

8 12 


)- v© 

30 a 


F19. 2-16 (a) A given series circuit, (b) A simpler equivalent circuit. 

it cannot be determined until R 3 is identified by removing it from the 
combination. It would have been better to have looked ahead and not made 
R 3 a part of the combination initially. 

An inspection of the Kirchhoff voltage equation for a series circuit also 
shows two other possible simplifications. The order in which elements are 
placed in a series circuit makes no difference, and several voltage sources 
in series may be replaced by an equivalent voltage source having a voltage 
equal to the algebraic sum of the individual sources. There is usually little 
advantage in including a dependent voltage source in a series combination. 

These simplifications may be illustrated by considering the circuit shown 
in Fig. 2- 16a. We first interchange the element positions in the circuit, 
being careful to preserve the proper sense of the sources, and then combine 
the three voltage sources into an equivalent 90-V source and the four 
resistors into an equivalent 30-fi resistance, as shown in Fig. 2-16b. Thus, 
instead of writing 

-80 + lOt - 30 + 7i + 5i + 20 + 8« = 

we have simply 


-90 + 30« = 
i = 3 A 

In order to calculate the power delivered to the circuit by the 80-V 
source appearing in the given circuit, it is necessary to return to that circuit 

Fig. 2-17 («) A circuit containing N parallel resistors having con- 
ductances Gj, G 2 , . . . , C s . [b) A simpler equivalent circuit: 

G„ = G l + G 2 + ■ ■ ■ + G x . 


43 Experimental Lows and Simple Circuits 

with the knowledge that the current is 3 A. The desired power is 240 W. 
It is interesting to note that no element of the original circuit remains 
in the equivalent circuit, unless we are willing to count the interconnecting 
wires as elements. 

Similar simplifications can be applied to parallel circuits. 3 A circuit 
containing N conductances in parallel, as in Fig. 2-17a, leads to the Kirch- 
. hoff current law equation, 

h = h + »2 + • • • + »w 
or i s = G t v + G 2 v + ■■■ + G N v = (G 1 + G 2 + ■ ■ ■ + G N )v 

whereas its equivalent in Fig. 2-l7b gives 

h = G e„ v 

and thus 

G eq = G 1 + G 2 + • • • + G N 

In terms of resistance instead of conductance, 

^L = J- + J-+ ...+J- 

01 Req = \/Ry + 1/R 2 + ■ • • + VR N 

This last equation is probably the most often used means of combining 
parallel resistive elements. 

The special case of only two parallel resistors 

1 __Rjfi2_ 

e " ~ l/R t + 1/R 2 ° r "> ~ R t + R 2 

is needed very often. The last form is worth memorizing. 

Parallel current sources may also be combined by algebraically adding 
the individual currents, and the order of the parallel elements may be 
rearranged as desired. 

The various combinations described in this section are used to simplify 
the circuit of Fig. 2-18a. Let us suppose that we wish to know the power 
and voltage of the dependent source. We may just as well leave it alone, 
then, and combine the remaining two sources into one 2-A source. The 
resistances are combined by beginning with the parallel combination of 
the two 6-J2 resistors into a 3-fi resistance, followed by the series combi- 

3 Duality. 

15 n< 

6 A 

f T O.DiV > > 

en< e n< 


Fig. 2-18 

[a] A given circuit, [b) A simplified equivalent circuit. 

nation of 3 and 15 0. The 18-0 and 9-0 elements combine in parallel 
to produce 6 0, and this is as far as we can proceed profitably. Certainly 
6 in parallel with 3 is 2 0, but the current t 3 on which the source 
depends then disappears. 4 

From the equivalent circuit in Fig. 2-18fc, we have 

-0.9i 3 -2 + t, + -£=0 



t; = 3i, 

i 3 = 10/3 A 
v = 10 V 

Thus, the dependent source furnishes (0.9)( 1 %)(10) = 30 W to the remain- 
der of the circuit. 

Now if we are belatedly asked for the power dissipated in the 15-0 
resistor, we must return to the original circuit. This resistor is in series 
with an equivalent 3-0 resistance; a voltage of 10 V is across the 18-0 total; 
thus, a current of % A flows through the 15-0 resistor and the power 
absorbed by this element is (%) 2 (15), or 4.63 W. 

To conclude the discussion of parallel and series element combinations, 
we should consider the parallel combination of two voltage sources and 
the series combination of two current sources. For instance, what is the 
equivalent of a 5-V source in parallel with a 10-V source? By the definition 
of a voltage source, the voltage across the source cannot change; by 
Kirchhoff's voltage law, then, 5 equals 10 and we have hypothesized a 
physical impossibility. Thus, voltage sources in parallel are permissible only 
when each has the same terminal voltage at every instant. Later, we shall 
see that practical voltage sources may be combined in parallel without any 
theoretical difficulty. 

4 Of course, we could have preserved it by using the given circuit to write i 3 = o/3, thus 
expressing i 3 in terms of variables appearing in the final circuit. 


45 ExpwimanM Laws and Simple Circuits 

In a similar way, two current sources may not be placed in series unless 
each has the same current, including sign, for every instant of time. 

A voltage source in parallel or series with a current source presents 
an interesting little intellectual diversion. *The two possible cases are 
illustrated by Prob. 29 at the end of the chapter. 

Drill Problems 

2-10 Find R eQ for the network of Fig. 2- 19a: (a) as it is shown; (b) with the 
5-0 resistor replaced by a short circuit (0 0); (c) with the 5-0 resistor replaced 
by an open circuit (oo 12). 

Arts. 9.933; 10; 10.2 




o w/v- 



.10 (2 





16 mU 

12 mU 

3 mU 

2 mU< 

,10 mU 

Fig. 2-19 See Drill Probs. 2-10 and 2-11. 

2-1 1 Find G eq for the network of Fig. 2-19fo: (a) as it is shown; (b) if it is 
disconnected and the six elements reconnected in parallel; (c) if it is disconnected 
and the six elements reconnected in series. 

Am. 0.830; 6; SI mO 

2-1 2 Find v x in the circuits of Fig. 2-20a, b, and c. 
2-13 Find i„ in the circuits of Fig. 2-20a, b, and c. 

Am. -60; 6; 48 V 

Am. -2; 0.5; 5 A 

o.i a 0.5 o 

i ^A> — f Wr 

Q f& 4A (b}> l°- 25a l«-*o I"" 



18 Q 

3 3«> 12v(±) 8fi< 8^ 



Fig. 2-20 See Drill Probs. 2-12 and 2-13. 


By combining resistances and sources, we have found one method of 
shortening the work of analyzing a circuit. Another useful shortcut is the 
application of the ideas of voltage and current division. 

Voltage division occurs when a dependent or independent voltage source 
is connected in series with two resistors, as illustrated in Fig. 2-21. The 
voltage across R 2 is obviously 

R t + R 2 

Fig. 2-21 An illustration of voltage division, v 2 = 

fi! + fl 2 

fl x + R 2 


I — w- 


12 sin t \(f) 6 0* 


Fig. 2-22 A numerical example illustrating resistance combination and voltage 
division. The wavy line within the source symbol indicates a sinusoidal variation 
with time. 

and the voltage across flj is, similarly, 

«! + R 2 

The voltage appearing across either of the series resistors is the applied 
voltage times the ratio of that resistance to the total resistance. Voltage 
division and resistance combination may both be applied, as in the circuit 
shown in Fig. 2-22. We mentally combine the 3- and 6-Q resistances, 
obtaining 2 S2, and thus find that v x is % of 12 sin t, or 4 sin t V. 

The dual of voltage division is current division. We now are given a 
current source in parallel with two conductances, as exemplified by the 
circuit of Fig. 2-23. The current flowing through G 2 is 

i2 = ^ = G * gTTgI 


and, similarly, 

' 2 ~ G 1 + G 2 l 

■ G i ■ 

Thus the current flowing through either of the parallel conductances 
is the applied current times the ratio of that conductance to the total 

Fig. 2-23 An illustration of current division. 




48 The Resistive Circuit 

Since we are given the value of the resistance more often than the 
conductance, a more important form of the last result is obtained by 
replacing G x by 1/R 1 and G 2 by l/fi 2 > 

Rl , . R2 ■ 
1 and " — • 

* R ± + fl 2 J «! + R 2 

Nature has not smiled on us here, for these last two equations have a factor 
which differs subtly from the factor used with voltage division, and some 
effort is going to be needed to avoid errors. Many students look on the 
expression for voltage division as "obvious" and that for current division 
as being "different." It also helps to realize that the larger resistor always 
carries the smaller current. 

As an example of the use of both current division and resistance combi- 
nation, let us return to the example of Fig. 2-22 and write an expression 
for the current through the 3-S2 resistor. The total current flowing into 
the 3- and 6-fi combination is 

, _ 12 sin t 

4 + (6)(3)/(6 + 3) 
and thus the desired current is 

. _ 12 sin t 6__ 

3 4 + (6)(3)/(6 + 3) 6 + 3 

= */ 3 sin t 


□ 1 For a section of conducting material of uniform cross-sectional area A, length 
I, and conductivity o (?5/m) or resistivity p (p = l/o, in S2-m), the resistance of 
the section is R = 1/oA = pi/ A. The resistivity of copper varies as a function 
of the absolute temperature T (100° < T < 500°K) as: p = 1.724 X 10" 8 [1 + 
0.00393(7 - 273)] fi-m. (a) Find the resistance of a 1000-turn coil of wire, average 
radius 4 cm, wire radius 1.4 X 10~ 2 cm, at 273°K. (b) By what percentage does 
the resistance increase as the temperature increases 100 °C? (c) If the total power 
dissipated in this coil is limited to 2 W, what is the maximum current it can carry? 

□ 2 If the resistance of a copper wire is proportional to its length and inversely 
proportional to its area, by what factor is the resistance increased when the same 
mass of material is used to produce a wire of: (a) twice the length? (b) half the 

□ 3 For the network shown in Fig. 2-24a, find i, v s , R, and the power supplied 
by the voltage source. 

Fig. 2-24 (a) See Prob. 3. [b) See Prob. 4. 

□ 4 For the circuit shown in Fig. 2-24fc, find v, i, and the power absorbed by 
element X. 

□ 5 If i, = 4 A and K = 3 £2 in the circuit of Fig. 2-25a, find the power absorbed 
by each of the five circuit elements. 

Fig. 2-25 (a] See Prob. 5. (fc) See Prob. 6. 

□ 6 If v y = 12 V and G = % U in the circuit of Fig. 2-256, find the power 
absorbed by each of the five circuit elements. 

□ 7 A circuit contains four nodes lettered A, B, C, and D. There are six branches, 
one between each pair of nodes. Let i AB be the current in branch AB directed 
from node A to node B through the element. Then, given i AS = 16 mA, and 
'da = 39 mA > And i AC , i BC , and i BD if i CD = : (a) 23 mA; (b) -23 mA. 

□ 8 A circuit contains six nodes lettered A, B, C, D, E, and F. Let u AB be the 
voltage between nodes A and B with its positive reference at the first-named node, 
here A. Find v AC , v AD , v AE , and v AF if v AB = 6 V, v BD = -3V,o c ,= -8 V, 
v EC = 4 V, and: (a) t> CJe = 1 V; (b) v CD = 1 V; (c) u ra = 4 V. 

□ 9 A series loop contains the following circuit elements in order: a 6-V source, 
a 2-kfi resistor, a 3-kK resistor, an 18-V source, and a 7-kfi resistor. The voltage 
sources aid. (a) Find the magnitude of the voltage across each resistor, (b) 
Determine the power absorbed by each element. 


50 The Resistive Circuit 

D 10 A 12-V battery is connected to a 5.5-0 load through wiring having a 
total resistance of 0.5 8. Find: (a) p load ; (b) p wiring \ (c) the total power supplied 
by the source; (d) efficiency = p load /{p load + PwiHng)- 

nil Specify i, v, and the power absorbed by the unknown circuit element in Fig. 
2-26o if the 100-V source supplies: (a) 100 W; (b) 300 W. 

2 X KTi, 

60 V 

<«> <«" 

Fig. 2-26 (a] See Probs. 11 and 12. (b) See Probs. 13 and 14. 

□ 12 In the circuit of Fig. 2-26a, consider the unknown element as a voltage 
source. What value should v be so that a charge of 600 C is delivered to the 
100-V source in 1 min? 

□ 1 3 (a) In the circuit shown in Fig. 2-26fc, find i v (b) Replace the dependent 
source by a 2-kfl resistor and again find i v 

□ 14 In the circuit shown in Fig. 2-26b, relabel the dependent source I3v v where 
v x is the voltage across the 1-kU resistor, positive reference at the left terminal 
of the resistor. Find i v 

□ 15 The following circuit elements are connected between a pair of nodes: a 
2-mU conductance, a 6-mA source, a 3-mJ5 conductance, an 18-mA source, and 
a 7-mtS conductance. The current sources are both directed into the upper node. 
(a) Find the magnitude of the current through each conductance, (b) Determine 
the power absorbed by each element. 

□ 1 6 Specify v, i, and the power absorbed by the unknown circuit element in Fig. 
2-27o if the 0.1-A source supplies: (a) 1 W; (b) 3 W. 

Fig. 2-27 (a) See Probs. 16 and 17. (fo] See Probs. 18 and 19. 

0.1 A 

2 X 10" OJ 4 mA 

8X 10" 

5 7 Experimental Laws and Simple Circuits 

D 17 In the circuit of Fig. 2-27 'a, consider the unknown as a current source. What 
would be the value of i if an energy of 120 J is delivered to the 0.1-A source in 
0.5 min? 

□ 18 (a) In the circuit of Fig. 2-27b, find t^. (b) Replace the dependent source 
by a 500-fi resistor and again find v v 

□ 19 In the circuit shown in Fig. 2-27fo, relabel the dependent source 13^, where 
ij is the downward current through the 10~ 3 -a conductance. Find v v 

□ 20 Find the power delivered to each of the 10-fi resistors in the circuit of Fie 

30 a 


0.1 A 

200 a 

160 n 26 a 


Fig. 2-28 (<z| See Prob. 20. (6) See Probs. 2! and 22 


□ 2 1 By combining resistances in the circuit of Fig. 2-2Sb, find the power supplied 
by the source and also the power absorbed by the 900-fi resistor. 

□ 22 The destruction (by open circuit) of which resistor in the circuit of Fig. 2-28Z> 
would cause the greatest increase in the power supplied by the current source? 
What is this power? 

□ 23 In the circuit shown in Fig. 2-29a, it is known that v 1 = 6 V. Find i s 
and v. 

Fig. 2-29 (a) See Probs. 23, 24, ond 25. [b) See Probs. 26 and 27. 

3 a 

— T WV 1 


52 The Resistive Circuit 

□ 24 In parallel with the independent current source in Fig. 2-29a, install a 
dependent current source, directed to the right, and labeled 0.6UJ. Find v t and 
the voltage v across both sources if i s is given as 12 A. 

□ 25 If i, = 4 A in the circuit of Fig. 2-29<z, calculate in a single step (each) the 
current, voltage, and power associated with the 342 resistor. 

□ 26 (a) Given i x = 1 A in the circuit of Fig. 2-29fc, find i and v,. (b) Use the 
results of (a) to determine i x if v s = 70 V; (c) if v s = 100 V. 

□ 27 Let v, = 50 V in the circuit of Fig. 2-29b. Using the concepts of voltage 
division, current division, and resistance combination, write a single expression 
that will yield the current i x . 

□ 28 What must be the resistance of R in the circuit of Fig. 2-30a? 

Fig. 2-30 (a) See Prob. 28. (b) See Prob. 29. 

D 29 (a) Find the power absorbed by each element in the circuit of Fig. 2-30fc. 
(b) How would the results change if the 2-Q resistor were reduced to 0? 

□ 30 Assume that the heating element for an electric hotplate consists of three 
concentric circles of resistance wire having radii of 2, 4, and 6 cm. Assume further 
that an ideal 230-V (dc) source is connected to diametrically opposite points on 
each ring. It is desired to provide a power of 10 W/cm length on every ring. 
Find the total source current and the resistance per unit length for each ring. 









v -■■■■■ •■■■ ^wi^iSif^'^lw^ ; -v- ■ • 'i.A^W'^^^^^S^mmmm 

, practicing i^; ^im.^l!^^ae$tfc^Me3ira(^fe^.t^^^^ 
^ . ' useful to Ij^^g^ ^aBftfe j^^> ftfag fandsneshifei 

54 "■• R**<*Kve Circuit 

coming years will include electric and electronic control circuits, commu- 
nication systems, energy converters such as motors and generators, power 
distribution systems, and entertainment or other devices which are now 
unknown. Many of us will be confronted with allied problems involving 
heat flow, fluid flow, and the behavior of various mechanical systems. In 
the analysis of any of these cases it is often helpful to replace the system 
with an equivalent electric circuit. As an example, we might consider a 
transistor amplifier, an electronic device which is a part of many commu- 
nication systems and control circuits. The transistor, along with several 
resistors and other passive circuit elements, is used to amplify or magnify 
an electrical signal and to direct the amplified signal to a desired load. 
It is possible to replace the transistor, the resistors, the other passive circuit 
elements, the signal source, and the load by combinations of simple circuit 
elements, such as current sources, voltage sources, and resistors. The 
solution of the problem is then achieved by circuit methods and techniques 
which we either know already or will meet in this chapter. 

When we are able to describe mathematically the behavior of fluid-flow 
and heat-flow systems, the dynamic response of aircraft control surfaces, 
and other nonelectrical phenomena, we shall see that the resultant equations 
are often precisely analogous to those describing current and voltage 
relationships in electric circuits. We may decide, then, that it is much easier 
and cheaper to construct the analogous electric circuit than it is to build 
a prototype of the actual physical system. The electric circuit may then 
be used to predict the performance of the other system as various elements 
are changed and may help achieve a better final design. This is the basis 
on which the electronic analog computer operates. 

It is evident that one of the primary goals of this chapter must be 
learning methods of simplifying the analysis of more complicated circuits. 
Among these methods will be superposition, loop, mesh, and nodal analysis. 
We shall also try to develop the ability to select the most convenient 
analysis method. Most often we are interested only in the detailed per- 
formance of an isolated portion of a complex circuit; a method of replacing 
the remainder of the circuit by a greatly simplified equivalent is then very 
desirable. The equivalent is often a single resistor in series or parallel with 
an ideal source. Thevenin's and Norton's theorems will enable us to do 

We shall begin studying methods of simplifying circuit analysis by 
considering a powerful general method, that of nodal analysis. 


In the previous chapter we considered the analysis of a simple circuit 
containing only two nodes. We found then that the major step of the 
analysis was taken as we obtained a single equation in terms of a single 

55 Some Useful Technique* of Circuit Analysis 

unknown quantity, the voltage between the pair of nodes. We shall now 
let the number of nodes increase, and correspondingly provide one addi- 
tional unknown quantity and one additional equation for each added node. 
Thus, a three-node circuit should have two unknown voltages and two 
equations; a ten-node circuit will have nine unknown voltages and nine 
equations; and an N-node circuit will need (N — 1) voltages and (N — 1) 

We consider the mechanics of nodal analysis in this section, but the 
justification for our methods will be developed toward the end of this 

As an example, let us consider the three-node circuit shown in Fig. 3-la. 
We may emphasize the locations of the 3 nodes by redrawing the circuit, 
as shown in Fig. 3-lfc, in which each node is identified by a number. 
We would now like to associate a voltage with each node, but we must 
remember that a voltage must be defined as existing between two nodes 
in a network. We thus select one node as a reference node, and then define 
a voltage between each remaining node and the reference node. Hence, 
we note again that there will be only (N — 1) voltages defined in an JV-node 

We choose node 3 as the reference node. Either of the other nodes 
could have been selected, but a little simplification in the resultant equa- 

3 A 

Reference node Ref. 

(c) (d) 

Fig. 3-1 (a) A given three-node circuit, [b] The circuit is redrawn to empha- 
size the three nodes, and each node is numbered, (c) A voltage, including 
polarity reference, is assigned between each node and the reference node. 
[d) The voltage assignment is simplified by eliminating the polarity references; 
it is understood that each voltage is sensed positive relative to the reference 

56 The Resistive Circuit 

tions is obtained if the node to which the greatest number of branches is 
connected is identified as the reference node. In some practical circuits 
there may be a large number of elements connected to a metallic case or 
chassis on which the circuit is built; the chassis is often connected through 
a good conductor to the earth. Thus, the metallic case may be called 
"ground," and this ground node becomes the most convenient reference 
node. More often than not, it appears as a common lead across the bottom 
of a circuit diagram. 

The voltage between node 1 and the reference node 3 is identified as 
v ± , and v 2 is defined between node 2 and the reference. These two voltages 
are sufficient, and the voltage between any other pair of nodes may be 
found in terms of them. For example, the voltage of node 1 with respect 
to node 2 is (v x — v 2 ). The voltages v x and v 2 and their reference signs 
are shown in Fig. 3-lc. In this figure the resistance values have also been 
replaced with conductance values. 

The circuit diagram is finally simplified in Fig. 3-ld by eliminating all 
voltage reference symbols. A reference node is plainly marked, and the 
voltages placed at each remaining node are understood to be the voltage 
of that node with respect to the reference node. 

We must now apply Kirchhoff's current law to nodes 1 and 2. We do 
this by equating the total current leaving the node through the several 
conductances to the total source current entering the node. Thus, 

0.5^ + 0.2(1)! - t> 2 ) = 3 
or OJuj - 0.2o 2 = 3 (1) 

At node 2 we obtain 

v 2 + 0.2(u 2 - Uj) = 2 
or -0.2^ + 1.2u 2 = 2 (2) 

Equations (1) and (2) are the desired two equations in two unknowns, 
and they may be solved easily. The result is: 

t?! = 5 V 

Also, the voltage of node 1 relative to node 2 is (t^ — v 2 ), or 2.5 V, and any 
current or power in the circuit may now be found in one step. For example, 
the current directed downward through the 0.5-0 conductance is 0.51^, or 
2.5 A. 

Now let us increase the number of nodes by one. A new circuit is shown 
in Fig. 3-2a, and it is redrawn in Fig. 3-2fc, with the nodes identified, a con- 

-3 A 




Fig. 3-2 (a) A circuit containing four nodes and eight branches. (&) The 
same circuit redrawn with node voltages assigned. 

venient reference node chosen, and the node voltages specified. We next sum 
the currents leaving node 1: 

3(«! - v 2 ) + 4( Vl - v a ) - (-8) - (-3) = 

7v x - 3u 2 - 4u 3 = -11 


At node 2: 

3(u 2 - V] ) + lv 2 + 2(o 8 - v 3 ) - 3 = 



and at node 3: 

4 ( v 3 ~ v i) + 2(«; 3 - v 2 ) + 5v 3 - 25 = 
— 4v 1 — 2v 2 + llu 3 = 25 


Equations (3) through (5) may be solved by a simple process of elimination 
of variables, or by Cramer's rule and determinants. 1 Using the latter method, 
we have 



















1 Appendix 1 provides a short review of determinants and the solution of a system of 
simultaneous linear equations by Cramer's rule. 


58 Trle Resistive Circuit 

Expanding the numerator and denominator determinants by minors along 
their first columns leads to 



-3 -4 



+ 25 

-3 -41 
6 -2 1 

J 6 - 2 I , „J -3-41 , ,J -3 -41 
1-2 lll-H-2 lll + H 6 -2 1 

-11(62) - 3(-41) + 25(30) -682 + 123 + 750 

7(62) + 3(-41) - 4(30) 


1 V 

434 - 123 - 120 























= 2 V 

= 3 V 

The denominator determinant is common to each of the three evalua- 
tions above. For circuits that do not contain either voltage sources or 
dependent sources (i.e., circuits containing only independent current 
sources), this denominator determinant may be written as a matrix 2 and 
defined as the conductance matrix of the circuit: 

G = 

7 -3 -4 
-3 6 -2 
-4 -2 11. 

It should be noted that the nine elements of the matrix are the ordered 
array of the coefficients of (3), (4), and (5), each of which is a conductance 
value. The first row is composed of the coefficients of the KirchhofF current 
law equation at the first node, the coefficients being given in the order 
of v v v 2 , and v 3 . The second row applies to the second node, and so on. 

2 There is no appendix on matrices because we shall not rely on matrix equations or matrix 
operations in this book. These topics, however, will certainly appear later in every engineer's 
professional courses as well as somewhere in his mathematics sequence. We shall identify 
the important matrices of circuit theory as we meet them. 


fig. 3-3 The 2-£5 conductance in the circuit of Fig. 3-2 is replaced by an 
independent voltage source. Kirchhoff's current law is used on the supernode 
enclosed by the broken line, and the source voltage is set equal to v 3 — v 2 . 

The conductance matrix is symmetrical about the major diagonal (upper 
left to lower right). This is a general consequence of the systematic way 
in which we assigned variables, applied Kirchhoff's current law, and ordered 
the equations, as well as of the reciprocity theorem, which we shall discuss 
in Chap. 16. For the present, we merely acknowledge the symmetry in 
these circuits that have only independent current sources and accept the 
check that it provides us in discovering errors we may have committed 
in writing circuit equations. 

We still must see how voltage sources and dependent sources affect 
the strategy of nodal analysis. We now investigate the consequences of 
including a voltage source. 

As a typical example, consider the circuit shown in Fig. 3-3. Our 
previous four-node circuit has been changed by replacing the 2-U conduct- 
ance between nodes 2 and 3 by a 22- V voltage source. We still assign 
the same node-to-reference voltages, o x , v 2 , and v 3 . Previously, the next 
step was the application of Kirchhoff's current law at each of the three 
nonreference nodes. If we try to do that once again, we see that we shall 
run into some difficulty at both nodes 2 and 3, for we do not know what 
the current is in the branch with the voltage source. There is no way by 
which we can express the current as a function of the voltage, for the 
definition of a voltage source is exactly that the voltage is independent 
of the current. 

There are two ways out of these difficulties. The more difficult is to 
assign an unknown current to the branch with the voltage source, proceed 
to apply Kirchhoff's current law three times, and then apply Kirchhoff's 
voltage law once between nodes 2 and 3; the result is four equations in 
four unknowns for this example. 

The easier method is to agree that we are primarily interested in the 
node voltages, so that we may avoid utilizing the voltage-source branch 
that is causing our problems. We do this by treating node 2, node 3, and 
the voltage source together as a sort of supernode and applying Kirchhoff's 


60 The Resistive Circuit 

current law to both nodes at the same time. This is certainly possible, 
because, if the total current leaving node 2 is zero and the total current 
leaving node 3 is zero, then the total current leaving the totality of the 
two nodes is zero. 

A simple way of considering the two nodes at the same time is to think 
of the voltage source as a short circuit physically joining the two nodes 
together. Thus, each voltage source will effectively reduce the number 
of nonreference nodes at which we must apply Kirchhoff's current law by 
one, regardless of whether the voltage source extends between two non- 
reference nodes or is connected between a node and the reference. 

So, let us visualize the 22-V source as a short circuit joining nodes 2 
and 3 together. We find six branches connected to this supemode (suggested 
by a broken line in Fig. 3-3). Beginning with the 3-0 conductance branch 
and working clockwise, we sum the six currents leaving this supernode: 

3(o 2 — Oj) — 3 + 4(c 3 - cj - 25 -(- 5u 3 + lc 2 = 
or — 7v t + 4to 2 + 9c 3 = 28 

The Kirchhoff current law equation at node 1 is unchanged from (3): 

lv 1 — 3c 2 — 4c 3 


We need one additional equation since we have three unknowns, and it 
must utilize the fact that there is a 22-V voltage source between nodes 
2 and 3, 


Rewriting these last three equations, 

7c! — 3c 2 — 4c 3 = — 11 
— 7o 1 -I- 4c 2 -(- 9c 3 = 28 
— c 2 + v 3 = 22 

the determinant solution for v 1 is 




















= -4.5 V 

Fig. 3-4 The 2-W conductance in the circuit of Fig. 3-2 is replaced by a 
dependent voltage source. The region within the broken line is treated as a 
supernode and the voltage i x /B is expressed as 4(u 3 — UjJ/8 and equated 
to v, — tv 

Note the lack of symmetry in the denominator determinant. This is 
a result of the presence of the voltage source. Note also that it would not 
make much sense to call the denominator determinant the conductance 
matrix of the circuit, for the bottom row comes from the equation 
— « 2 + t> 3 = 22, and this equation does not depend on any conductances 
in any way. 

Now let us include a dependent source. We again replace the 2-U 
conductance in Fig. 3-2, this time by a dependent voltage source, as 
indicated in Fig. 3-4. We select a dependent voltage source rather than 
a dependent current source, as we have found that voltage sources offer 
us more of a challenge than do current sources in nodal analysis. Further- 
more, we let the dependent source be controlled by a current rather than 
by a voltage, because this also is the less easy of the two cases to analyze. 

In Fig. 3-4 then, the dependent voltage source is i x /8, where »„ is the 
current toward the left in the 4-U conductance. The same three node-to- 
reference voltages are selected, and, since we again do not know the current 
in the dependent source branch, we let nodes 2 and 3 and the source be 
a supernode for which Kirchhoff 's current law again yields * 

3 («2 - »i) ~ 3 + 4 (« 3 - »i) - 25 + 5v 3 + lv 2 = 
or -7cj + 4v 2 + 9v 3 = 28 

At node 1 

~tv x — 3v 2 — 4v 3 = — 11 

which is also unchanged. Turning our attention finally to the dependent 
source, we have 


52 The Itotktive Circuit 


8 8 

or — 0.5OJ + v 2 — 0.5u 3 = 

With determinants, v 1 is 









u l 











= 1 V 

This result happens to be the same as that for the original four-node cir- 
cuit (Fig. 3-2), as are the values for v 2 and v 3 . 

Let us summarize the method by which we may obtain a set of nodal 
equations for any resistive circuit: 

1 Make a neat, simple, circuit diagram. Indicate all element and 
source values. Conductance values are preferable to resistance 
values. Each source should have its reference symbol. 

2 Assuming that the circuit has N nodes, choose one of these nodes 
as a reference node. Then write the node voltages v lt o 2 , . . . , v N _ 1 
at their respective nodes, remembering that each node voltage is 
understood to be measured with respect to the chosen reference. 

3 If the circuit contains only current sources, apply Kirchhoff 's current 
law at each nonreference node. To obtain the conductance matrix 
if a circuit has only independent current sources, equate the total 
current leaving each node through all conductances to the total 
source current entering that node, and order the terms from v x to 
%_!■ For each dependent current source present, relate the source 
current and the controlling quantity to the variables v v v 2 , ■ ■ ■ , 
%_i, if they are not already in that form. 

4 If the circuit contains voltage sources, mentally replace each such 
source by a short circuit, thus reducing the number of nodes by 
one, and apply Kirchhoff's current law at each of this reduced 
number of nodes. Relate the source voltage to the variables v v 
v 2 , . . . , %_!> if it is not already in that form. 

With these suggestions in mind, let us consider the circuit displayed 
in Fig. 3-5, one which contains all four types of sources and has five nodes. 

fig. 3-5 A five-node circuit containing all of the four different types of sources. 

We select the central node as the reference, and assign v 1 to « 4 in a 
clockwise direction starting from the left node. 

After thinking of each voltage source as a short circuit, we see that 
we need to write Kirchhoff 's current law equations only at node 2 and 
at the supernode containing both nodes 3 and 4 and the dependent voltage 

At node 2, 

2(f 2 

1 (u 2 - v 3 ) 

while at the supernode, 

l(v 3 - v 2 ) - 2,v x + 2v 4 + l(v 4 -v 1 ) = 
We next relate the source voltages to the node voltages: 

v 1= -1 

v 3 - t) 4 = 4o„ = 4(v 4 - Vl ) 

And finally we express the dependent current source in terms of the assigned 

2 Cl = 2(o 2 - Cl ) 

Thus, we obtain four equations in the four node voltages: 

— 2cj + 3v 2 — v 3 = 2 

t> 1= -1 
v i ~ 3v 2 + v 3 + 3t> 4 = 

4t) l + v 3 — 5°4 = 


£4 The Resistive Circuit 

to which the solutions are 

Cj = - 1 V 

»2= 17 / 9 V 

»3 = 1 % V 

«4 = ys v 

Drill Problems 

3-1 In the circuit of Fig. 3-6, use nodal analysis to find: (a) v A ; (b) v B ; (c) v c . 

Ans. -2.5; 4.5; 7 V 

4 1i< "c ( f ) 24 A. 

0.8 « 

Fig. 3-6 'See Drill Probs. 3-1, 3-2, 3-3, and 3-4. 

3-2 Replace the 24-A source in Fig. 3-6 with a dependent current source, with 
the upward-directed arrow labeled — 6i B , where i B is the downward current in 
the 0.8-15 conductance. Find: (a) v A ; (b) v B ; (c) v c . 

Ans. - 2 %; 4 %; 71 / 7 V 

3-3 Replace the 24-A source in Fig. 3-6 with a 22-V voltage source, positive 
reference at the top, and find: (a) v A ; (b) v B ; (c) u c . 

Ans. 10; 12; 22 V 

3-4 Replace the 24-A source in Fig. 3-6 with a dependent voltage source, positive 
reference at the bottom, labeled 0.6c B . Find: (a) v A ; (b) v B ; (c) v c . 

Ans. -4; 2.4; 6.4 V 


The technique of nodal analysis described in the preceding section is 
completely general and can always be applied to any electrical network. 
This is not the only method for which a similar claim can be made, 

Fig. 3-7 (a) A planar network can be drawn on a plane surface without 
crossovers, [b) A nonplanar network cannot be drawn on a plane surface 
without at least one crossover, (c) A planar network can be drawn so that 
it may look nonplanar. 

however. In particular, we shall meet a generalized nodal analysis method 
and a technique known as loop analysis in the concluding sections of this 

First, however, let us consider a method known as mesh analysis. Even 
though this technique is not applicable to every network, it can be applied 
to most of the networks we shall need to analyze, and it is widely used. 
Mesh analysis is applicable only to those networks which are planar, a term 
we now proceed to define. 

If it is possible to draw the diagram of a circuit on a plane surface 
in such a way that no branch passes over or under any other branch, then 
that circuit is said to be a planar circuit. Thus, Fig. 3-7a shows a planar 
network, Fig. 3-7fc shows a nonplanar network, and Fig. 3-7c shows a planar 
network, although it is drawn in such a way as to make it appear nonplanar 
at first glance. 

In the first chapter, a circuit was defined as a network containing at 
least one closed path about which current might flow. The official name 
for this closed path is a loop. Thus, if we begin at" a certain node and 
trace a continuous closed path through the network, passing through no 
node or element more than once and ending at the same node, that path 
is a loop. Figure 3-8 shows several examples. The particular paths con- 
sidered are those which are drawn with heavy lines, and it is evident that 
the first two paths cannot be loops since the path either is not closed or 
passes through a node twice. The remaining four paths are all loops. The 
circuit contains 11 branches. 

The mesh is a property of a planar circuit and is not defined for a 
nonplanar circuit. We define a mesh as a loop which does not contain any 
other loops within it. Thus, the loops indicated in Fig. 3-8c and d are not 
meshes, whereas those of e and / are meshes. This circuit contains four 

If a network is planar, mesh analysis can be used to accomplish its 



(rf) (e) 

Fig. 3-8 (a) The path identified by the heavy line is not a loop since it 
is not closed, (b) The path here is not a loop since it passes through the central 
node twice, (c) This path is a loop but not a mesh since it encloses other 
loops, [d) This path is also a loop but not a mesh, (e) and (/) Each of these 
paths is both a loop and a mesh. 

analysis. This technique involves the concept of a mesh current, which 
we shall introduce by considering the analysis of the two-mesh circuit of 
Fig. 3-9. 

As we did in the single-loop circuit, we shall begin by assuming a current 
through one of the branches. Let us call the current flowing to the right 
through the 6-Q resistor i v We intend to apply Kirchhoff's voltage law 
around each of the two meshes, and the resulting two equations are suffi- 
cient to determine two unknown currents. Therefore we select a second 
current i 2 flowing to the right in the 4-fi resistor. We might also choose 
to call the current flowing downward through the central branch i 3 , but 
it is evident from Kirchhoff's current law that » 3 may be expressed in terms 
of the two previously assumed currents as (tj — i 2 ). The assumed currents 
are shown in Fig. 3-9. 

Fig. 3-9 Two currents, i x and t 2 , are assumed in a two-mesh circuit. 

42 v(+) 


67 So" 1 * Useful Technique* of Circuil Analysis 

Following the method of solution for the single-loop circuit, we now 
apply Kirchhoff 's voltage law to the left-hand mesh, 

-42 + 6JJ + 3(»! - i 2 ) = 
or 9^ - 3i 2 = 42 (6) 

and then to the right-hand mesh, 

-3(ij - i 2 ) + 4i 2 - 10 = 
or -3ij + 7i 2 = 10 (7) 

Equations (6) and (7) are independent equations; one cannot be derived 
from the other. 3 There are two equations and two unknowns, and the 
solution is easily obtained: i t is 6 A, i 2 is 4 A, and (ij — tg) is therefore 
2 A. The voltage and power relationships may be quickly obtained if 

If our circuit had contained M meshes, then we should have had to 
assume M branch currents and write M independent equations. 4 The 
solution in general may be systematically obtained through the use of 

Now let us consider this same problem in a slightly different manner 
by using mesh currents. We define a mesh current as a current which flows 
only around the perimeter of a mesh. If we label the left-hand mesh of 
our problem as mesh 1, then we may establish a mesh current i x flowing 
in a clockwise direction about this mesh. A mesh current is indicated by 
a curved arrow that almost closes on itself and is drawn inside the appro- 
priate mesh, as shown in Fig. 3-10. The mesh current t 2 is established in 
the remaining mesh, again in a clockwise direction. Although the direction 
.is arbitrary, we shall always choose clockwise mesh currents because a 
certain error-minimizing symmetry then results in the equations. 

We no longer have a current or current arrow shown directly on each 

« v 

Fig. 3-10 A clockwise mesh current is assigned to each mesh of a planar 

Ht will be shown in Sec. 3-8 that mesh equations are always independent. 
*The proof of this statement will be found in Sec. 3-8. 

£g The Resistive Circuit 

branch in the circuit. The current through any branch must be determined 
by considering the mesh currents flowing in every mesh in which that 
branch appears. This is not difficult because it is obvious that no branch 
can appear in more than two meshes. For example, the 342 resistor appears 
in both meshes, and the current flowing downward through it is (i x — i 2 ). 
The 6-S2 resistor appears only in mesh 1, and the current flowing to the 
right in that branch is equal to the mesh current i v 

A mesh current may often be identified as a branch current, as i t and 
i 2 are identified above. This is not always true, however, for consideration 
of a square nine-mesh network soon shows that the central mesh current 
cannot be identified as the current in any branch. 

One of the greatest advantages in the use of mesh currents is the fact 
that Kirchhoff's current law is automatically satisfied. If a mesh current 
flows into a given node, it obviously flows out of it also. 

We therefore may turn our attention to the application of Kirchhoff's 
voltage law to each mesh. For the left-hand mesh, 

-42 + 6j x + 3(i t - i 2 ) = 

while for the right-hand mesh, 

3(» 2 - ij) + 4i 2 - 10 = 

and these two equations are the same as (6) and (7). 

Let us next consider the five-node, seven-branch, three-mesh circuit 
shown in Fig. 3-11. The three required mesh currents are assigned as 
indicated, and we methodically apply Kirchhoff's voltage law about each 

-7 + lft - i 2 ) + 6 + 2ft - » 3 ) = 

l(i 2 - i t ) + 2i 2 + 3(i 2 - i 3 ) = 

2(i 3 - i x ) - 6 + 3(i 3 - i 2 ) + li 3 = 

fig. 3-11 Mesh currents i v i^, and i 3 are assumed in a five-node seven- 
branch three-mesh circuit. 

7 V 


£9 $° m * Useful Techniques of Circuit Analysis 


-ij + 6i 2 — 3i 3 = 
-2tj - 3i 2 + 6t 3 = 6 

and Cramer's rule leads to the formulation for u 









H — 











= 3 A 

The other mesh currents are i x — 3 A, and i 2 — 2 A. 

Again we notice that we have a denominator determinant that is 
symmetrical about the major diagonal. This occurs for circuits that contain 
only independent voltage sources when clockwise mesh currents are 
assigned, where the elements appearing in the first row of the determinant 
are the ordered coefficients of i v i 2 , . . . , i M in the Kirchhoff voltage law 
equation about the first mesh, where the second row corresponds to the 
second mesh, and so on. This symmetrical array appearing in the denomi- 
nator determinant is termed the resistance matrix of the network, 

R = 










How must we modify this straightforward procedure when a current 
source is present in the network? Taking our lead from nodal analysis (and 
duality), we should feel that there are two possible methods. First, we could 
assign an unknown voltage across the current source, apply Kirchhoff's 
voltage law around each mesh as before, and then relate the source current 
to the assigned mesh currents. This is generally the more difficult approach. 

A better technique is the dual of the supernode approach of nodal 
analysis. Instead of short-circuiting voltage sources to create supernodes, 
thus reducing the total number of nodes, we now open-circuit or remove 
current sources to create loops ("supermeshes"), thereby reducing the total 
number of meshes. We apply Kirchhoff's voltage law only to those meshes 
in the modified network. 

1 fi. 

7V ©0 r 

7 A( 





fig. 3-12 Mesh analysis is applied to this circuit containing a current source 
by writing the Kirchhoff-voltage-law equation about the loop: 7 V, 1 Q, 3 fi 

1 a. 

As an example of this procedure, consider the network shown in Fig. 
3-12, in which a 7-A independent current source is in the common boundary 
of two meshes. Mesh currents i lt i 2 , and i 3 are assigned, and the current 
source is mentally open-circuited, thus creating a new mesh whose interior 
is that of meshes 1 and 3. Applying Kirchhoff's voltage law about this 

-7 + 1(h - i 2 ) + 3(i 3 - i 2 ) + 1« 3 = 
h ~ 4 »2 + 4i 3 = 7 


and around mesh 2, 

l(i 2 - h) + 2i 2 + 3(i 2 - » 3 ) = 
or -tj + 6t 2 - 3i 3 = 

Finally, the source current is related to the assumed mesh currents, 

»i - H = 7 
Solving (8) through (10), we have 




L 6 


L -4 






L 6 


I -4 




28.-2 A 
14 - 2 A 

We may also find that tj = 9 A and t 2 = 2.5 A. 


1 U 

Fig. 3-13 The presence of two current sources in this three-mesh circuit mokes 
it necessary to apply Kirchhoff's voltage law only once, around mesh 2. 

The presence of one or more dependent sources merely requires each 
of these source quantities and the variable on which it depends to be 
expressed in terms of the assigned mesh currents. In Fig, 3-13, for example, 
we note that both a dependent and an independent current source are 
included in the network. Three mesh currents are assigned and Kirchhoff's 
voltage law is applied to mesh 2: 

1(» 2 - i t ) + 2i 2 + 3(t 2 - « 3 ) = 

The current sources appear in meshes 1 and 3; when they are open- 
circuited, only mesh 2 remains, and we already have an equation for it. 
We therefore turn our attention to the source quantities, obtaining 


i x = 15 

%v* = h ~ »i = VMh ~ h)] 


-i x + 6i 2 - 3i 3 = 
i t = 15 

-h + y 3 *2 + %h = ° 

from which we have i x — 15, t 2 = 11, and i 3 = 17 A. We might note that 
we wasted a little time in assigning a mesh current i t to the left mesh; 
we should simply have indicated a mesh current and labeled it 15 A. 

Let us summarize the method by which we may obtain a set of mesh 
equations for a resistive circuit: 

1 Make certain that the network is a planar network. If it is nonplanar, 
mesh analysis is not applicable. 

2 Make a neat, simple, circuit diagram. Indicate all element and 


72 The Resistive Circuit 

source values. Resistance values are preferable to conductance 
values. Each source should have its reference symbol. 

3 Assuming that the circuit has M meshes, assign a clockwise mesh 
current in each mesh, i lt i 2 , . . . , i M . 

4 If the circuit contains only voltage sources, apply Kirchhoff 's voltage 
law around each mesh. To obtain the resistance matrix if a circuit 
has only independent voltage sources, equate the clockwise sum of 
all the resistor voltages to the counterclockwise sum of all the source 
voltages, and order the terms from i t to i M . For each dependent 
voltage source present, relate the source voltage and the controlling 

quantity to the variables i v i 2 
that form. 

i M , if they are not already in 

If the circuit contains current sources, mentally replace each such 
source by an open circuit, thus reducing the number of meshes by 
one, and apply Kirchhoff 's voltage law around the meshes of the 
resultant network. Relate the source current to the variables « 1 , 
t 2 , . . . , i M , if it is not already in that form. 

Drill Problems 

3-5 In the circuit of Fig. 3-14, use mesh analysis to find: (a) i A ; (b) i B ; (c) i c . 

Ans. -%; 1; % mA 

21 V 

12 kS! 

Fig. 3-14 See Drill Probs. 3-5, 3-6, 3-7, and 3-8. 

3-6 Replace the 28-V source in Fig. 3-14 by a dependent voltage source, positive 
reference on the left, labeled 21,000t B . Find: (a) i A \ (b) i B ; (c) i c . 

Ans. -3; -%; 13 / 3 mA 

3-7 Replace the 6-kfi resistor of Fig. 3-14 with a 4-mA current source, reference 
arrow directed upward, and find: (a) i A ; (b) i B ; (c) i c . 

Ans. - u / 3 ; -y 3 ,- 4 mA 

3-8 Replace the 3-kB resistor of Fig. 3-14 with a dependent current source, arrow 
directed to the right, labeled 500i c . Find: (a) i A ; (b) i B ; (c) i c . 

Ans. -2; %; % mA 

73 Some Useful Techniques of Circuit Analysis 


In all our previous work we have been making continual use of ideal voltage 
and current sources; it is now time to take a step closer to reality by 
considering practical sources. These sources will enable us to make more 
realistic representations of physical devices. Having defined the practical 
sources, we shall then study methods whereby practical current and voltage 
sources may be interchanged without affecting the remainder of the circuit. 
Such sources will be called equivalent sources. Our methods will be 
applicable for both independent and dependent sources. 

The ideal voltage source was defined as a device whose terminal voltage 
is independent of the current through it. A 1-V dc source produces a 
current of 1 A through a 1-U resistor and a current of 1,000,000 A through 
a 1-fiQ resistor; it may provide an unlimited amount of power. No such 
device exists practically, of course, and we agreed that a real physical source 
might be represented by an ideal source only as long as relatively small 
currents, or powers, were drawn from it. For example, an automobile 
storage battery may be approximated by an ideal dc voltage source if its 
current is limited to a few amperes. However, anyone who has ever tried 
to start an automobile with the headlights on must have observed that the 
lights dimmed perceptibly when the battery was asked to deliver the heavy 
starter current, 100 A or more, in addition to the headlight current. Under 
these conditions, an ideal voltage source may be a very poor representation 
of the storage battery. 

The ideal voltage source must be modified to account for the lowering 
of its terminal voltage when large currents are drawn from it. Let us 
suppose that we observe experimentally that a storage battery has a termi- 
nal voltage of 12 V when no current is flowing through it and a reduced 
voltage of 11 V when 100 A is flowing. Thus, a more accurate repre- 
sentation might be an ideal voltage source of 12 V in series with a resistor 
across which 1 V appears when 100 A flows through it. The resistor must 
be 0.01 Q, and the ideal voltage source and this series resistance comprise 
a practical voltage source. This particular practical voltage source is 
shown connected to a general load resistor R L in Fig. 3-15a; the terminal 
voltage of the practical source is the same as the voltage across R L and 
is marked v L . In Fig. 3-15b a plot of the terminal voltage as a function 
of the load resistance points out the fact that the output voltage approaches 
that of the ideal source only for large values of the load resistance where 
relatively small currents are drawn. The terminal voltage is only one-half 
the voltage of the ideal source when the load resistance is equal to the 
internal resistance of the practical source. 

Let us now consider a general practical voltage source, as shown in 
Fig. 3-16. The voltage of the ideal source is v s , and a resistance R sv , called 
an internal resistance, is placed in series with it. The resistor is not one 

Fig. 3-15 (a) A practical source which approximates the behavior of a cer- 
tain 12-V storage battery is shown connected to a load resistor R L . (b) The 
terminal voltage decreases as R L decreases and i L increases. 

which we would wire or solder into a circuit, but merely serves to account 
for a terminal voltage which decreases as the load current increases, and 
thus its presence enables us to represent a physical voltage source more 
closely. The voltage v L across the load resistor R L is thus 

~TK* L 


and the load current i L is 

R >„ + R r. 


An ideal current source is also nonexistent in the real world; there is 
no physical device which will deliver a constant current, regardless of the 
load resistance to which it is connected or the voltage across its terminals. 
A pentode vacuum-tube amplifier and certain transistor circuits will deliver 
a constant current to a wide range of load resistances, but the load resistance 
can always be made sufficiently large that the current through it becomes 
very small. Infinite power is simply never available. 

Fig. 3-16 A general practical vokage source connected to a load resistor R L . 


Fig. 3-17 (a) A general practical current source connected to a load resistor 
R L . {b) The load current provided by the practical current source is shown 
as a function of the load resistance. 

A practical current source is defined as an ideal current source in 
parallel with an internal resistance R si . Such a source is shown in Fig. 
3-17a, and the current i L and voltage v L produced across a load resistor 
R L are indicated. It is apparent that 


R.< . 

R« + «/. 


The variation of load current with changing load resistance is shown in 
Fig. 3-17fe, and it is evident that the load current and ideal source current 
are approximately equal only for values of load resistance which are small 
compared with R si . 

Having defined both practical sources, we are now ready to discuss their 
equivalence. We shall define two sources as being equivalent if each 
produces identical current and identical voltage in any load which is placed 
across its terminals. In other words, if we are confronted with two black 
boxes, each having a single pair of terminals on it, then there is no way 
in which we can differentiate between the boxes by measuring current or 
voltage in a resistive load. 

It should be noted carefully that although equivalent sources will deliver 
the same current, voltage, and power to identical resistive loads, the power 
which the two ideal sources supply and the power absorbed in R sv and 
R $i may be quite different. 

The conditions for equivalence are now quickly established. Since the 
load currents are to be identical, from (12) and (14) we have 

K s „ + «l R 8i + «L 


2 n 

3 A 



Fig. 3-18 (a) A given practical current source, [b] The equivalent practical 
voltage source: R tv = R si = R„ : v, = R,i,. 

and if these two expressions are to be the same for any R L , then it follows 

R*„ — A«i = R. 



where we shall now let R s represent the internal resistance of either 
practical source. It is easily shown that these same two conditions may 
be obtained from (11) and (13). 

As an example of the use of these ideas, consider the practical current 
source shown in Fig. 3-18a. Since its internal resistance is 2 Q, the internal 
resistance of the equivalent practical voltage source is also 2 $2; the voltage 
of the ideal voltage source contained within the practical voltage source 
is (2)(3) = 6 V. The equivalent practical voltage source is shown in Fig. 

To check the equivalence, let us visualize a 4-fl resistor connected to 
each source. In both cases, a current of 1 A, a voltage of 4 V, and a power 
of 4 W are associated with the 4-12 load. However, the ideal current source 
is delivering a total power of 12 W, while the ideal voltage source is 
delivering only 6 W. Correspondingly different powers are dissipated in 
the two internal resistances. 

It is enlightening to develop the equivalence conditions by a slightly 
different method. Suppose that we are given a practical current source 
and are asked to determine the equivalent voltage source. There are two 
unknowns, v s and R tv . We therefore need two facts, or equations, and we 
may easily obtain these by forcing the current that each source delivers 
to a short circuit and the voltage that each delivers to an open circuit to 
be identical. We first equate the two short-circuit currents 

"> ~ R. 

and, hence, 


"Jf Some Useful Techniques of Circuit Analysis 

and then the two open-circuit voltages 


and v. — R.i, 

as before. 

A very useful power theorem may be developed with reference to a 
practical voltage or current source. For the practical voltage source (Fig. 
3-16 with R sv = R s ), the power delivered to the load R L is 

., 2n 

Pl = k 2 R 

L "t 

(«. + «l)' 

To find the value of R L that absorbs a maximum power from the given 
practical source, we differentiate with respect to R L : 

dp L _ (ft. + R L )V - v, 2 R L (2)(R, + R L ) 
dR L (H. + R L ) 4 

and equate the derivative to zero, obtaining, 

2R L (R a + R L ) = (R, + R L f 
or R, = R L 

Since the values, R L = and R L — oo, both give a minimum (p L = 0), and 
since we have already developed the equivalence between practical voltage 
and current sources, we have therefore proved the following maximum 
power transfer theorem: 

An independent voltage source in series with a resistance R, or an independent 
current source in parallel with a resistance R s delivers a maximum power to 
that load resistance R L for which R L = R s . 

Drill Problems 

3-9 For the circuit shown in Fig. 3- 19a: (a) use nodal analysis to find the power 
supplied by the 3-A source; (b) transform the practical voltage source into a 
practical current source and use nodal analysis to find the power supplied by the 
new ideal current source; (c) transform the practical current source into a practical 

36 V 

Fi 9 . 3-19 See Drill Probs. 3-9 and 3-10. 

voltage source and use mesh analysis to find the power supplied by the new ideal 
voltage source. 

Ans. -48; 84; 504 W 

3-10 Find v x in the circuit shown in Fig. 3-19fc by: (a) nodal analysis; (b) mesh 
analysis; (c) beginning on the right side of the circuit and alternating source 
transformations and source and resistance combinations until only a single loop 
circuit remains. 

Am. %; %; % V 


All the circuits which we have analyzed up to now (and which we shall 
analyze later) are linear circuits. At this time we must be more specific 
in defining a linear circuit. Having done this, we can then consider the 
most important consequence of linearity, the principle of superposition. 
This principle is very basic and will appear repeatedly in our study of linear 
circuit analysis. As a matter of fact, the nonapplicability of superposition 
to nonlinear circuits is the reason they are so difficult to analyze. 

The principle of superposition states that the response (a desired current 
or voltage) at any point in a linear circuit having more than one inde- 
pendent source can be obtained as the sum of the responses caused by each 
independent source acting alone. In the following discussion, we shall 
investigate the meaning of "linear" and "acting alone." We shall also take 
note of a slightly broader form of the theorem. 

The difference between linearity and nonlinearity may first be illustrated 
by a nonelectrical example. Let us place one loaded truck (the forcing 
function) in the middle of a suspension bridge and measure the deflection 
(response) of the bridge. It turns out to be 3 cm. A second truck may 
produce another 3 cm, indicating a linear system, but if we try to extend 
the results too far we may extend the bridge too far. The system becomes 
nonlinear, and response is no longer proportional to force or excitation. 

Let us first define a linear element as a passive element that has a linear 
voltage-current relationship. By a "linear voltage-current relationship" we 
shall mean simply that multiplication of the time-varying current through 


79 Some Useful Techniques of Circuit Analysis 

the element by a constant K results in the multiplication of the time- varying 
voltage across the element by the same constant K. At this time, only one 
passive element has been defined, the resistor, and its voltage-current 

v(t) = Ri(t) 

is obviously linear. As a matter of fact, if v(t) is plotted as a function of 
i(t), the result is a straight line. We shall see in Chap. 4 that the defining 
voltage-current equations for inductance and capacitance are also linear 
relationships, as is the defining equation for mutual inductance presented 
in Chap. 15. 

We must also define a linear dependent source as a dependent current 
or voltage source whose output current or voltage is proportional only to 
the first power of some current or voltage variable in the circuit or to the 
sum of such quantities. That is, a dependent voltage source, v s = 
0.6^ — 14t> 2 , is linear, but v s — 0.6tj 2 and v t = 0.6iyV 2 are not. 

We may now define a linear circuit as a circuit composed entirely of 
independent sources, linear dependent sources, and linear elements. From 
this definition, it is possible to show 5 that "the response is proportional 
to the source," or that multiplication of all independent source voltages 
and currents by a constant K increases all the current and voltage responses 
by the same factor K (including the dependent source voltage or current 

The most important consequence of linearity is superposition. Let us 
prove the superposition principle by considering first the circuit of Fig. 
3-20, which contains two independent sources, the current generators which 
force the currents i a and ij into the circuit. Sources are often called farcing 
functions for this reason, and the voltages which they produce between 
node 1 or 2 and the reference node may be termed response functions, 
or simply responses. Both the forcing functions and the responses may 
be functions of time. 

The two nodal equations for this circuit are 

0.7UJ - 0.2u 2 = i a (17) 

-0.2^ + 1.2u 2 = tj (18) 

5 The proof involves first showing that the use of nodal analysis on the linear circuit can 
produce only linear equations of the form: 

ap^ + 0&2 + • • • + a w t>„ = b 

where the a t are constants (combinations of resistance or conductance values, constants 
appearing in dependent source expressions, 0, or ± 1), the v t are the unknown node voltages 
(responses), and & is an independent source value or a sum of independent source values. 
Given a set of such equations, if we multiply all the b's by K, then it is evident that the 
solution of this new set of equations will be the node voltages Kv l3 Kv 2 Kv„. 


Fig. 3-20 A three-node circuit containing two forcing functions used to 
illustrate the superposition principle. 

Now let us perform experiment x. We change the two forcing functions 
to i ax and i^; the two unknown voltages will now be different, and We 
shall let them be v lx and v 2x . Thus, 

0.7o„ - 0.2« 2l = i„ (19) 

-0.2€ lx + 1.2<; 2x = i 6l (20) 

We next perform experiment y by changing the source currents to i ay and 
i by and by letting the responses be v ly and v 2y , 

0.7*„ - 0.2 U2v = i„„ (21) 

-0.2c lv + 1.2o 2 , = ij„ (22) 

These three sets of equations describe the same circuit with different source 
currents. Let us add or superpose the last two sets of equations. Adding 

(19) to (21), 

(0.7 ClI + 0.7e lv ) - (0.2o 2l + 0.2t> 2lf ) = i„ + i at , (23) 

0.7 Ol - 0.2«; 2 = i a (17) 

and adding (20) to (22), 

-(0.2 ClI + 0.2o 11( ) + (1.2o 2l + 1.2o 2 „) = ij, + «„„ (24) 

-0.2 Ol + 1.2c 2 = ij (18) 

where (17) has been written immediately below (23), and (18) below (24) 
for easy comparison. 

The linearity of all these equations allows us to compare (23) with (17) 
and (24) with (18) and draw an interesting conclusion. If we select i ax and 
i ay such that their sum is i a , select i hx and i by such that their sum is %, then 
the desired responses t> x and v 2 may be found by adding v u to v ly and 
v 2x to v 2v , respectively. In other words, we may perform experiment x 
and note the responses, perform experiment y and note the responses, and 
finally add the corresponding responses. These are the responses of the 


3 1 Soma Utahl Techniques of Circuit Analysis 

original circuit to independent sources which are the sums of the inde- 
pendent sources used in experiments * and y. This is the fundamental 
concept involved in the superposition principle. 

It is evident that we may extend these results by breaking up either 
source current into as many pieces as we wish; there is no reason why 
we cannot perform experiments z and q also. It is only necessary that the 
algebraic sum of the pieces be equal to the original current. 

The superposition theorem usually appears in a form similar to the 

In any linear resistive network containing several sources, the voltage across 
or the current through any resistor or source may be calculated by adding 
algebraically all the individual voltages or currents caused by each inde- 
pendent source acting alone, with all other independent voltage sources 
replaced by short circuits and all other independent current sources replaced 
by open circuits. 

Thus if there are N independent sources, we perform N experiments. Each 
independent source is active in only one experiment, and only one inde- 
pendent source is active in each experiment. An inactive independent 
voltage source is identical with a short circuit, and an inactive independent 
current source is an open circuit. Note that dependent sources are in general 
active in every experiment. 

Our proof of superposition, however, should indicate that a much 
stronger theorem might be written; a group of independent sources may 
be made active and inactive collectively, if we wish. For example, suppose 
there are three independent sources. The theorem above states that we 
may find a given response by considering each of the three sources acting 
alone and adding the three results. Alternatively, we may find the response 
due to the first and second sources operating with the third inactive, and 
then add to this the response caused by the third source acting alone. This 
amounts to treating several sources collectively as a sort of supersource. 

There is also no reason that an independent source must assume only 
its given value or a zero value in the several experiments; it is only necessary 
for the sum of the several values to be equal to the original value. An 
inactive source almost always leads to the simplest circuit, however. 

Let us illustrate the application of the superposition principle by 
considering an example in which both types of independent source are 
present. It is not necessary to transform either source. For the circuit of 
Fig. 3-21, let us use superposition to write an expression for the unknown 
branch current i x . We may first kill the current source and obtain the 
portion of i x due to the voltage source as 0.2 A. Then if we kill the voltage 
source and apply current division, the remaining portion of i x is seen to 
be 0.8 A. We might write the answer in detail as 

i -2A 

Fig. 3-21 A circuit containing both an independent current and a voltage 
source which is easily analyzed by the superposition principle. 

h = <»li.=o + h 

-5— + 2— - 6 — = 0.2 + 0.8 = 1.0 A 

■*l».=o 6 + 9 6 + 9 

As an example of the application of the superposition principle to a 
circuit containing a dependent source, consider Fig. 3-22. We seek i z , and 
we first open-circuit the 3-A source. The single mesh equation is 

so that 

- 10 + 2l' x + \i' x + 2i' x = 

»: = 2 

Next, we short-circuit the 10-V source and write the single-node equation, 

v" v" — 2t" 

and relate the dependent-source-controlling quantity to v' 

v" = -2i" 

We find 
and, thus, 

i" = -0.6 

L - 2 - 0.6 = 1.4 

Fig. 3-22 Superposition may be used to analyze this circuit by first replacing 
the 3-A source by an open circuit and then replacing the 10-V source by a 
short circuit. The dependent voltage source is always active (unless t I — 0). 


83 *"•"• UMfal TachniquM of Circuit Analytic 

It usually turns out that little if any time is saved in analyzing a circuit 
containing one or more dependent sources by use of the superposition 
principle, for there must always be at least two sources in operation: one 
independent source and all the dependent sources. 

We must constantly be aware of the limitations of superposition. It 
is applicable only to linear responses, and thus the most common nonlinear 
response — power — is not subject to superposition. For example, consider 
two 1-V batteries in series with a 1-J2 resistance. The power delivered to 
the resistor is obviously 4 W, but if we mistakenly try to apply superposition 
we might say that each battery alone furnished 1 W and thus the total 
power is 2 W. This is incorrect. 

Drill Problems 

3-1 1 Use superposition to find v in each of the circuits shown in Fig. 3-23. 

Ans. -3; 4; 6 V 


6 V( 

6 V( 

4 n< 




o.5 n 
►o.6 n 


•0.4 n 


-21 A 

Fig. 3-23 See Drill Prob. 3-1 


120 mA 

3-1 2 First find v x in the circuit of Fig. 3-24 by using the superposition principle 
and then determine the power generated by: (a) the 5-A source; (b) the 6-V source; 
(c) the dependent source. 

Ans. -12.32; 14; 21.6 W 


6 V 
Fig. 3-24 See Drill Prob. 3-12. 


Now that we have the superposition principle, it is possible to develop 
two more theorems which will greatly simplify the analysis of many linear 
circuits. The first of these theorems is named after M. L. Thevenin, a 
French engineer working in telegraphy, who first published a statement 
of the theorem in 1883; the second may be considered a corollary of the 
first and is credited to E. L. Norton, a scientist with the Bell Telephone 

Let us suppose that we need to make only a partial analysis of a circuit; 
perhaps we wish to determine the current, voltage, and power delivered 
to a single load resistor by the remainder of the circuit, which may consist 
of any number of sources and resistances; or perhaps we wish to find the 
response for different values of the load resistor. Th6venin's theorem 
then tells us that it is possible to replace everything except the load resistor 
by an equivalent circuit containing only an independent voltage source 
in series with a resistor; the response measured at the load resistor will 
be unchanged. Using Norton's theorem, we obtain an equivalent composed 
of an independent current source in parallel with a resistor. 

It should thus be apparent that one of the main uses of Thevenin's 
and Norton's theorems is the replacement of a large part of a network, 
often a complicated and uninteresting part, by a very simple equivalent. 
The new, simpler circuit enables us to make rapid calculations of the 
voltage, current, and power which the original circuit is able to deliver 
to a load. It also helps us to choose the best value of this load resistance. 
In a transistor power amplifier, for example, the Thevenin or Norton 
equivalent enables us to determine the maximum power that can be taken 
from the amplifier and the type of load that is required to accomplish a 
maximum transfer of power or to obtain maximum practical voltage or 
current amplification. 

Consider the circuit shown in Fig. 3-25. The broken lines separate the 
circuit into networks A and B; we shall assume that our main interest is 
in network B, which consists only of the load resistor R L . Network A may 
be simplified by making repeated source transformations. We first treat the 


Network A Network B 

Fig. 3-25 A simple resistive circuit is divided into network A, in which we 
have no detailed interest, and network B, a load resistor with which we are 

12-V source and the 3-ft resistor as a practical voltage source and replace 
it with a practical current source consisting of a 4-A source in parallel with 
3 Q. The parallel resistances are then combined into 2 ft, and the practical 
current source which results is transformed back into a practical voltage 
source. The steps are indicated in Fig. 3-26, the final result appearing in Fig. 
3-26d. From the viewpoint of the load resistor R L , this circuit (the Thevenin 
equivalent) is equivalent to the original circuit; from our viewpoint, the 
circuit is much simpler and we can now easily compute the power delivered 
to the load. It is 

" = (9T«r) 2 ^ 

Furthermore we can see from the equivalent circuit that the maximum 
voltage which can be obtained across R L is 8 V; a quick transformation 

Hq. 3-26 The source transformations and resistance combinations involved 
in simplifying network A are shown in order. The result, given in (d), is the 
Thevenin equivalent. 

35 ^e Resistive Circuit 

of network A to a practical current source (the Norton equivalent) indicates 
that the maximum current which may be delivered to the load is % A; 
and the maximum power transfer theorem shows that a maximum power 
is delivered to R L when R L is 9 £2. None of these facts is readily apparent 
from the original circuit. 

If network A had been more complicated, the number of source trans- 
formations and resistance combinations necessary to obtain the Thevenin 
or Norton equivalent could easily become prohibitive. Thevenin's and 
Norton's theorems allow us to find the equivalent circuit much more quickly 
and easily, even in more complicated circuits. 

Let us now state Thevenin's theorem formally: 

Given any linear circuit, rearrange it in the form of two networks A and 
B that are connected together by two resistanceless conductors. Define a 
voltage v oc as the open-circuit voltage which would appear across the 
terminals of A if B were disconnected so that no current is drawn from A. 
Then all the currents and voltages in B will remain unchanged if A is killed 
(all independent voltage sources and independent current sources inA replaced 
by short circuits and open circuits, respectively) and an independent voltage 
source v oc is connected, with proper polarity, in series with the dead (inactive) 
A network. 

The terms killed and dead are a little bloodthirsty, but they are descrip- 
tive and concise, and we shall use them in a friendly way. Moreover, it 
is possible that network A may only be sleeping, for it may still contain 
dependent sources which come to life whenever their controlling currents 
or voltages are nonzero. 

Let us see if we can apply Thevenin's theorem successfully to the 
circuit we considered in Fig. 3-25. Disconnecting R L , voltage division 
enables us to determine that v oc is 8 V. Killing the A network, that is, 
replacing the 12-V source by a short circuit, we see looking back into 
the dead A network a 7-S2 resistor connected in series with the parallel 
combination of 6 Q and 3 0. Thus the dead A network can be represented 
here by simply a 9-£2 resistor. This agrees with the previous result. 

The equivalent circuit we have obtained is completely independent of 
the B network, because we have been instructed first to remove the B 
network and measure the open-circuit voltage produced by the A network, 
an operation which certainly does not depend on the B network in any 
way, and then to place the inactive A network in series with a voltage 
source v oc . The B network is mentioned in the theorem and proof only 
to indicate that an equivalent for A may be obtained; no matter what 
arrangement of elements is connected to the A network; the B network 
represents this general network. 

87 S°n>* Useful Techniques of Circuit Analysis 

A proof of Thevenin's theorem in the form in which we have stated 
it is rather lengthy, and therefore it has been placed in Appendix 2 where 
the curious or rigorous may peruse it. 

There are several points about the theorem which deserve emphasis. 
First, it is not necessary to impose any restrictions on A or B, other than 
requiring that the original circuit composed of A and B be a linear circuit. 
No restrictions were imposed on the complexity of A or B; either one may 
contain any combination of independent voltage or current sources, linear 
dependent voltage or current sources, resistors, or any other circuit elements 
which are linear. The general nature of the theorem (and its proof) will 
enable if to be applied to networks containing inductors and capacitors, 
which are linear passive circuit elements to be defined in the following 
chapter. At this time, however, resistors are the only passive circuit 
elements which have been defined, and the application of Thevenin's 
theorem to resistive networks is a particularly simple special case. The 
dead A network can be represented by a single equivalent resistance, R th . 

Norton's theorem bears a close resemblance to Thevenin's theorem, 
another consequence of duality. As a matter of fact, the two statements 
will be used as an example of dual language when the duality principle 
is discussed in the following chapter. 

Norton's theorem may be stated as follows: 

Given any linear circuit, rearrange it in the form of two networks A and 
B that are connected together by two resistanceless conductors. Define a 
current i sc as the short-circuit current which would appear at the terminals 
of A if B were short-circuited so that no voltage is provided by A. Then 
all the voltages and currents in B will remain unchanged if A is killed (all 
independent current sources and independent voltage sources in A replaced 
by open circuits and short circuits, respectively) and an independent current 
source i sc is connected, with proper polarity, in parallel with the dead (inactive) 
A network. 

If A is an active resistive network, then it is obvious that the inactive 
A network may be replaced by a single equivalent resistance, which we 
shall also call the TTieVenin resistance, since it is once again the resistance 
viewed at the terminals of the inactive A network. The Norton equivalent 
of an active resistive network is therefore the Norton current source i sc 
in parallel with the Thevenin resistance R th . 

There is an important relationship between the Thevenin and Norton 
equivalents of an active resistive network. The relationship may be ob- 
tained by applying a source transformation to either equivalent network. 
For example, if we transform the Norton equivalent, we obtain a voltage 
source R tk i sc in series with the resistance R th ; this network is in the form 

8 V 

1 kfi 

Fig. 3-27 (a) A given circuit in which the 1-kB resistor is identified as 
network B. (b) The Thevenin equivalent is shown for network A. (c) The 
Norton equivalent is shown for network A. 

of the Th6venin equivalent, and thus 

R thhi 


In resistive circuits containing dependent sources as well as independent 
sources, we shall often find it more convenient to determine either the 
Thevenin or Norton equivalent by finding both the open-circuit voltage 
and the short-circuit current and then determining the value of R th as their 
quotient. It is therefore advisable to become adept at finding both open- 
circuit voltages and short-circuit currents, even in the simple problems 
which follow. If the Th6venin and Norton equivalents are determined 
independently, (25) may serve as a useful check. 

Let us consider three examples of the determination of a Thevenin or 
Norton equivalent circuit. The first is shown in Fig. 3-27a; the Thevenin and 
Norton equivalents are desired for the network faced by the 1-kfi resistor. 
That is, network B is this resistor, and network A is the remainder of the given 

We first kill both independent sources to determine the form of the 
dead A network. With the 4-V source short-circuited and the 2-mA source 
open-circuited, the result is the series combination of a 2-kS2 and 3-Ml 
resistor, or the equivalent, a 5-kfi resistor. The open-circuit voltage is easily 
determined by superposition. With only the 4-V source operating, the 
open-circuit voltage is 4 V; when only the 2-mA source is on, the 
open-circuit voltage is also 4 V; with both independent sources operating, 
we see that v oc = 4 + 4 = 8 V. This determines the Thevenin equivalent, 
shown in Fig. 3-27b, and from it the Norton equivalent of Fig. 3-27c can 
be drawn quickly. As a check, let us determine t 8C for the given circuit. 


89 'Som« Useful Techniques of Circuit Analysis 

We use superposition and a little current division: 

he = *.cU V + *«c|2 nU = 2^-3 + 2 Y^J = - 8 + - 8 = L6 mA 

which completes the check. 

As the second example, we consider the network A shown in Fig. 3-28, 
which contains a dependent source. We desire the Thevenin equivalent. 
To find « oc we note that v x — v oc , and that the dependent source current 
must pass through the 2-kfl resistor since there is an open circuit to the 
right. Summing voltages around the outer loop: 

-4 + 2 X 10 3 (^g-) + 3 X mo) + v, = 
and v x = 8 = t> oc 

By Thevenin's theorem, then, the equivalent could be formed with the dead 
A network in series with an 8-V source, as shown in Fig. 3-28fc. This is 
correct, but is not very simple and not very helpful; in the case of linear 
resistive networks, we should certainly show a much simpler equivalent 
for the inactive A network, namely R th . We therefore seek i ac . Upon 
short-circuiting the output terminals in Fig. 3-28a, it is apparent that v x = 
and the dependent current source is zero. Hence, i K = 4/(5 X 10 3 ) = 

Fig. 3-28 (a) A given network whose Thevenin equivalent is desired, {b) 
A possible, but rather useless, form of the Thevenin equivalent, (c) The best 
form of the Thevenin equivalent for this linear resistive network. 

o.e n« 

Fig. 3-29 (a) A network, containing no independent sources, whose Thevenin 
equivalent is desired, (b) R th is numerically equal to v. (c] The Thevenin 
equivalent of (a). 

0.8 mA. Thus, R th = v oc /i sc = 8/(0.8 X 10" 3 ) = 10 kil, and the accepted 
Thevenin equivalent of Fig. 3-28c is obtained. 

As our final example, let us consider a network having a dependent 
source but no independent source, such as that shown in Fig. 3-29o. The 
network therefore qualifies already as the dead A network, and v oc = 0. 
We thus seek the value of R th represented by this two-terminal network. 
However, we cannot find v oc and i sc and take their quotient, for there is 
no independent source in the network and both v oc and i sc are zero. Let 
us, therefore, be a little tricky. We apply a 1-A source externally, measure 
the resultant voltage, and then set R th = v/1. Referring to Fig. 3-29fo, we 
see that i = — 1 and 

t,_i.5(-l) v „ 

J -I — =1 

3 2 

so that 

v = 0.6 V 


The Thevenin equivalent is shown in Fig. 3-29c. 

Although we are devoting our attention almost entirely to the analysis 
of linear circuits, it is enlightening to know that Thevenin's and Norton's 
theorems are both valid if network B is nonlinear; only network A must 
be linear. 


9 1 S»m* UmM Techniques of Circuit Analysis 

Drill Problems 

3-13 Find the Thevenin equivalent of the network shown in Fig. 3-30a if: (a) 
d = 0, C 2 = 12 V; (b) Cj = 0.2 A/V, C 2 = 12 V; (c) Cj = 0.2 A/V, C 2 = 0. 

Arts. V, 12.5 Q; 6 V, 5 Si; 15 V, 12.5 Q 




10 fl. 




1.27 n 7.18 a 


Fig. 3-30 See Drill Probs. 3-13 and 3-14. 

3-14 Find the Norton equivalent of the network to the left of terminals ab in 
Fig. 3-30& if element X is: (a) a 5-ti resistor; (b) a 3-A independent current source, 
arrow directed upward; (c) a dependent voltage source, labeled 2i v positive 
reference at top. 

Am. 0A,8 Q; A, 14 U; 2 A, 30 S2 


In this section we shall generalize the method of nodal analysis that we 
have come to know and love. Since this method is applicable to any general 
network, we cannot promise that we shall be able to solve a wider class 
of circuit problems. We can, however, look forward to being able to select 
a nodal analysis method for any particular problem that may result in fewer 
equations and less work. 

We must first extend our list of definitions relating to network topology. 
We begin by defining topology itself as a branch of geometry which is 
concerned with those properties of a geometrical figure which are un- 
changed when the figure is twisted, bent, folded, stretched, squeezed, or 
tied in knots, with the provision that no parts of the figure are to be cut 

— ' 

(«) (i) 

Fig. 3-31 (a) A given circuit, [b) The linear graph of this circuit. 

apart or to be joined together. A sphere and a tetrahedron are topologically 
identical, as are a square and a circle. In terms of electric circuits, then, 
we are not now concerned with the particular types of elements appearing 
in the circuit, but only with the way in which branches and nodes are 
arranged. As a matter of fact, we usually suppress the nature of the 
elements and simplify the drawing of the circuit by showing the elements 
as straight lines. The resultant drawing is called a linear graph, or simply 
a graph. A circuit and its graph are shown in Fig. 3-31. Note that all 
nodes are identified by heavy dots in the graph. 

Since the topological properties of the circuit or its graph are unchanged 
when it is distorted, the three graphs shown in Fig. 3-32 are all topologically 
identical with the circuit and graph of Fig. 3-31. 

Topological terms which we already know and have been using cor- 
rectly are: 

node: a point at which two or more elements have a common connec- 

branch: a single path, containing one simple element, which connects 
one node to any other node. 

Fig. 3-32 The three graphs shown are topologically identical to each other 
and to the graph of Fig. 3-31&, and each is a graph of the circuit shown 
in Fig. 3-3 la. 










Fig. 3-33 [a) The linear graph of a three-node network, [b), [c), [d), and 
[e] Four of the eight different trees which may be drawn for this graph are 
shown by the heavy tines. 

loop: a set of branches forming a closed path which passes through no 
node more than once. 

mesh: a loop which does not contain any other loops within it. 
planar circuit: a circuit which may be drawn on a plane surface in such 
a way that no branch passes over or under any other branch. 
nonplanar circuit: any circuit which is not planar. 

The graphs of Fig. 3-32 each contain 12 branches and 7 nodes. 

Two new properties of a linear graph must now be defined, a tree and 
a link. We may define a tree as any set of branches which does not contain 
any loops but which connects every node to every other node, not neces- 
sarily directly. There are usually a number of different trees which may 
be drawn for a network, and the number increases rapidly as the complexity 
of the network increases. The simple graph shown in Fig. 3-33a has eight 
possible trees, four of which are shown by heavy lines in Fig. 3-33fo, c, 
d, and e. 

In Fig. 3-34a a more complex graph is shown. Figure 3-34fo shows one 
possible tree, and Fig. 3-34c and d shows sets of branches which are not 
trees because neither set satisfies the definition above. 

Once we understand the construction of a tree, the concept of the link 
is very simple, for a link is any branch in a linear graph which is not a 
branch of the tree. It is evident that any particular branch may or may 
not be a link, depending on the particular tree which is selected. 

The number of links in a graph may be related to the number of 
branches and nodes very simply. If the graph has N nodes, then exactly 
(N — 1) branches are required to construct a tree because the first branch 
chosen connects two nodes and each additional branch includes one more 

Fig. 3-34 (a) A linear graph, (b) A possible tree for this graph. 
[d) These sets of branches do not satisfy the definition of a tree. 

I and 


94 Tr| e Resistive Circuit 

node. Thus, given B branches, the number of links L must be 

L = B-(N-1) 
or L = B - N + 1 (26) 

In any of the graphs shown in Fig. 3-33, we note that 3 = 5 — 3 + 1, 
and in the graph of Fig. 3-34fc, 6 = 10 — 5+1. A network may be in 
several disconnected parts, and (26) may be made more general by replacing 
+ 1 with + S, where S is the number of separate parts. However, it is also 
possible to connect two separate parts by a single conductor, thus causing 
two nodes to form one node; no current can flow through this single 
conductor. This process may be used to join any number of separate parts, 
and thus we shall not suffer any loss of generality if we restrict our attention 
to circuits for which S = 1. 

We are now ready to discuss a method whereby a set of nodal equations 
may be written for a network that are independent and sufficient. The 
method will enable us to obtain many different sets of equations for the 
same network, and all the sets will be valid. However, the method does 
not provide us with every possible set of equations. Let us first describe 
the procedure, illustrate it by an example, and then point out the reason 
that the equations are independent and sufficient. 

Given a network, we first draw its graph and then construct a tree. 
Any tree will do, and we shall see shortly how to choose that tree which 
is most convenient for our purposes. We next focus our attention on the 
branches in the tree. Each tree branch is assigned a voltage, extending 
from the node at one end of the tree branch to the other. Thus, there 
are (N — 1) voltages chosen since the tree contains (N — 1) branches. Kirch- 
hoff 's current law is then applied to any (N — 1) nodes, and the remaining 
node may be ignored. This corresponds to the presence of the reference 
node in our previous attack on nodal analysis. The equation written at 
the iVth node is not independent; it may be obtained from the other (N — 1) 

If there are voltage sources in the network, they should be placed in 
the tree and the source voltage should be assigned as that tree-branch 
voltage. Any dependent source that is voltage controlled should have that 
control voltage placed in a tree branch if possible. Current sources should 
be placed in links, and currents that control dependent sources should also 
be placed in links whenever possible. 

In applying Kirchhoff 's current law at (N — 1) nodes, it is evident that 
we cannot express the current of any voltage source in terms of the source 
voltage; hence, we again mentally replace each voltage source by a short 
circuit and form supernodes at which Kirchhoff 's current law is applied. 
Thus, each voltage source will result in the (N — 1) Kirchhoff current law 
equations being one less in number. 



y- 1 v 





+ > 

<«> (6) 

Fig. 3-3S (a) The circuit of Fig. 3-5 repeated, (b) A tree is chosen such 
that both voltage sources and both control voltages are tree branches. 

The procedure may be illustrated by considering an example we ana- 
lyzed earlier by denning all node voltages with respect to a reference node. 
The circuit is that of Fig. 3-5, repeated as Fig. 3-35a. We draw a tree 
so that both voltage sources and both control voltages appear as tree-branch 
voltages and, hence, as assigned variables. As it happens, these four 
branches constitute a tree, Fig. 3-35b, and tree-branch voltages v x , 1, v , 
and 4t3„ are chosen, as shown. 

Considering both voltage sources as short circuits, we apply Kirchhoff's 
current law twice, once to the top node, 

2v x + l(o x -v v - 4c,) = 2 

and once to the supernode consisting of the right node, the bottom node, 
and the dependent voltage source, 

lv v + 2(o, - 1) + 1(40, + 

»*) = 2o, 

Instead of the four equations we had previously, we have only two, and 
we find easily that v x = 2 % V and v y — % V, both values agreeing with 
the earlier solution. 

Now let us discuss the sufficiency of the assumed voltages and the 
independence of the nodal equations. If these tree-branch voltages are 
sufficient, then every branch voltage must be obtainable from a knowledge 
of the values of all the tree-branch voltages. Once every branch voltage 
is known, it is apparent that every branch current or power can be readily 
obtained and thus the tree-branch voltages will be "sufficient" information 
to enable a complete solution to be obtained if desired. But we certainly 
can express every branch voltage in terms of the tree-branch voltages. This 
is already accomplished for those branches in the tree. For the links, we 
know that each link extends between two nodes, and, by definition, the 
tree must also connect those two nodes. Hence, every link voltage may 


9(3 The Resistive Circuit 

also be established in terms of the tree-branch voltages. Thus, sufficiency 
is demonstrated. 

To show that the (2V — 1) nodal equations are independent, visualize the 
application of Kirchhoff 's current law to the (N — 1) different nodes. Each 
time we write the Kirchhoff current law equation, there is a new tree 
branch involved — the one which connects that node to the remainder of 
the tree. Since that circuit element has not appeared in any previous 
equation, we must obtain an independent equation. This is true for each 
of the (N — 1) nodes in turn, and hence we have (N — 1) independent equa- 

Drill Problem 

3-15 By constructing a suitable tree, rework part (b) of Drill Prob.: (a) 3-1, using 
only two equations; (£>) 3-3, using only one equation; (c) 3-4, using only one 

Arts. -4; -2.5; 10 V 


Now we shall consider the use of a tree to obtain a suitable set of loop 
equations. In some respects this is the dual of the method of writing nodal 
equations. Again it should be pointed out that, although we are able to 
guarantee that any set of equations we write will be both sufficient and 
independent, we should not expect that the method will lead directly to 
every possible set of equations. 

We begin by constructing any convenient tree for the given network 
and then focus our attention on any arbitrary link. If that link is added 
to the tree, a closed loop must be formed; to this loop we assign our first 
loop current. It flows through certain branches in the tree and through 
this particular link. Now let us temporarily ignore that first link and the 
first loop current. We select another link, imagine its addition to the tree, 
note that once again a loop is formed, and assign our second loop current 
to this loop. The process is repeated for each link and, since there are 
(B — N + 1) links, we end up with (B — N + 1) loop currents; no link has 
more than one loop current flowing in it. We thus may describe the current 
interchangeably as a link current or a loop current. The procedure is now 
familiar; Kirchhoff 's voltage law is applied to each loop, as defined by its 
loop current, and the resultant equations may be solved by determinants, 
substitution, inspection, or digital computer. 

If there are current sources in the network, they should be placed in 
the links and the source current should be assigned as that link current. 
Any dependent source that is current controlled should have that control 

97 Some Useful Technique! of Circuit Analysis 

current placed in a link, if possible. Voltage sources should be placed in 
tree branches, and voltages that control dependent sources should also be 
placed in tree branches whenever possible. Note that the general rule either 
for nodal analysis or loop analysis is to place voltages in tree branches and 
currents in links, a mandatory rule for sources and a desirable rule for 
controlling quantities. 

In applying Kirchhoff 's voltage law around (B — N + 1) loops, it is 
evident that we cannot express the voltage of any current source in 
terms of the source current; hence, we again replace each current source 
mentally by an open circuit, thus discarding the loop that would be 
formed by the closure of that link. Each current source therefore results in 
the (B — N + 1) Kirchhoff voltage law equations being one less in number. 

Let us illustrate this procedure by reworking an earlier example solved 
by mesh currents. The circuit is shown in Fig. 3-12 and redrawn in Fig. 
3-36a. The tree is selected so that the voltage source is in a tree branch 
while the current source is in a link, Fig. 3-36£>. Upon closing the short, 
central, vertical link, a loop (also mesh) current is established and labeled 
7 A. This link is opened and the short, central, horizontal link is closed; 
the resultant loop current is also a mesh current, and it is called i A . This 
link is opened and the last link is closed, permitting a loop current to be 
present around the perimeter of the circuit, i B . Note that in each case 
the closure of the link defines only one loop current that is present in tree 
branches and that link only. 

The equation about the i A loop is 

and for the i B loop, 

l(i A - 7) + 2(i A + i B ) + 3i A = 

-7 + 2(i A +i B ) + \i B = 

Fig. 3-36 (a) The circuit of Fig. 3-1 2 is shown again, (b) A tree is chosen 
such that the current source is in a link and the voltage source is in a tree 


i n< 

*« n 


7 A 


'i n 



7 A 1 




Fig. 3-37 A tree which is used as an example to illustrate the sufficiency 
of the link currents. 

and we have i A — 0.5 A, i B = 2 A, as before. The solution was achieved 
with one less equation than before. 

How may we demonstrate sufficiency? Let us visualize a tree. It 
contains no loops and therefore contains at least two nodes to each of which 
only one tree branch is connected. The current in each of these two 
branches is easily found from the known link currents by applying Kirch- 
hoff 's current law. If there are other nodes at which only one tree branch 
is connected, these tree-branch currents may also be immediately obtained. 
In the tree shown in Fig. 3-37, we thus have found the currents in branches 
a, b, c, and d. Now we move along the branches of the tree, finding the 
currents in the tree branches e and /; the process may be continued until 
all the branch currents are determined. The link currents are therefore 
sufficient to determine all branch currents. It is helpful to look at the 
situation where an incorrect "tree" has been drawn which contains a loop. 
Even if all the link currents were zero, a current might still circulate about 
this "tree loop." Hence, the link currents could not determine this current, 
and they would not represent a sufficient set. Such a "tree" is by definition 

In order to demonstrate that the (B — N + 1) loop equations are inde- 
pendent, it is only necessary to point out that each represents the appli- 
cation of Kirchhoff 's voltage law around a loop which contains one link 
not appearing in any other equation. We might visualize a different 
resistance R t , R 2 , . . . , R B _ N+1 in each of these links, and it is then apparent 
that one equation can never be obtained from the others since it contains 
one coefficient not appearing in any other equation. 

Hence, the link currents are sufficient to enable a complete solution 
to be obtained, and the set of loop equations which we use to find the 
link currents is a set of independent equations. 

Having looked at both general nodal analysis and loop analysis, we 
should now consider the advantages and disadvantages of each method so 
that an intelligent choice of a plan of attack can be made. 

The nodal method in general requires (N — 1) equations, but this num- 
ber is reduced by one for each independent or dependent voltage source 


4 sin 10001 mV ' 


Fig. 3-38 A sinusoidal voltage source and a 10-kfl load are connected to 
the T-equivalent circuit of a transistor. The common connection between the 
input and output is at the base terminal of the transistor and the arrangement 
is called the common-base configuration. 

in a tree branch, and increased by one for each dependent source that is 
voltage controlled by a link voltage or current controlled. 

The loop method basically involves (B — N + 1) equations. How- 
ever, each independent or dependent current source in a link reduces this 
number by one, while each dependent source that is current controlled 
by a tree-branch current or is voltage controlled increases the number 
by one. 

As a grand finale for this discussion, let us inspect the T-equivalent- 
circuit model for a transistor, shown in Fig. 3-38, to which are connected 
a sinusoidal source, 4 sin 1000* mV, and a 10-kft load. We select typical 
values for the emitter resistance, r e = 50 0; for the base resistance, r t = 
500 £2; for the collector resistance, r c = 20 k£2; and for the common-base 
forward-current-transfer ratio, a = 0.98. Suppose that we wish to find the 
input (emitter) current i e and the load voltage v L . 

Although the details are requested in Drill Probs. 3-17 and 3-18 below, 
we should see readily that the analysis of this circuit might be accomplished 
by drawing trees requiring three general nodal equations (N — 1 — 1 + 1) 
or two loop equations (B — N + 1 — 1). We might also note that three 
equations are required in terms of node-to-reference voltages, as are three 
mesh equations. 

No matter which method we choose, these results are obtained for this 
specific circuit: 

i e = 18.1 sin lOOOf juA 
v L = 120 sin lOOOf mV 

and we therefore find that this transistor circuit provides a voltage gain 
(v L /v s ) of 30, a current gain (t3 £ /10,000i e ) of 0.659, and a power gain equal 
to the product, 30(0.659) = 19.8. Higher gains could be secured by oper- 
ating this transistor in a common-emitter configuration, as illustrated by 
Prob. 30. 


1 00 The R«i*<ive Circuit 

Drill Problems 

3-16 By constructing an appropriate tree, rework: (a) part (b) of Drill Prob. 3-5, 
using only two equations; (b) part (c) of Drill Prob. 3-7, using only one equation; 
(c) part (c) of Drill Prob. 3-8, using only one equation. 

Arts. -%,• _y„. % A 

3-17 For the transistor amplifier equivalent circuit shown in Fig. 3-38, let 
r e = 50 fi, r t = 500 Q, r c = 20 \sSl, a = 0.98, and find both i e and v L by drawing 
a suitable tree and using: (a) two loop equations; (b) three nodal equations with 
a common reference node for the voltages; (c) three nodal equations without a 
common reference node. 

Arts. 18.1 sin lOOOt pA and 120 sin lOOOt mV 

3-18 Determine the Thevenin and Norton equivalent circuits presented to the 
10-kS2 load in Fig. 3-38 by finding: (a) the open-circuit value of v L ; (b) the 
(downward) short-circuit output current; (c) the Thevenin equivalent resistance. 
AIL circuit values are given in Drill Prob. 3-17. 

Arts. 146 sin lOOOt mV; 65.6 sin lOOOt fiA; 2230 Q 


□ 1 In Fig. 3-39, let circuit element X be a 2-U conductance. Find the power 
supplied by the 10-A source. 

Fi(|. 3-39 See Probs. 1 to 4. 

□ 2 In Fig. 3-39, let circuit element X be a 10-V source with its positive voltage 
reference at the upper right node. Find the power supplied by the 10-A current 

□ 3 In Fig. 3-39, let circuit element X be a dependent voltage source with its 
positive voltage reference at the right node and having a voltage of t^/3, where 
the 10-A source supplies a power 10%. Find v v 

101 So™* Useful Techniques of Circuif Analysis 

D 4 In Fig. 3-39, circuit element X is a dependent current source, 40^3, with 
the reference arrow directed toward the upper right node. Let the power supplied 
by the 10-A source be lOt^; find v t . 

□ 5 For the circuit shown in Fig. 3-40a: (a) let R = 4 Q and use nodal methods 
to find the power supplied by the 7-A source; (b) repeat if R is infinite. 

14 A 

Fig. 3-40 See Probs. 5 and 6. 

□ 6 With reference to Fig. 3-40fc, let the lower node be the reference, and write 
the single nodal equation required to find v,. How much power is delivered by 
the dependent source? 

□ 7 In Fig. 3-41, let circuit element X be a 2-fl resistance. Find the power supplied 
by the 6-V source. 

12 v 

Fig. 3-41 See Probs. 7 to 10. 

□ 8 In Fig. 3-41, let circuit element X be a 6-A source with its arrow directed 
to the right. Find the power supplied by the 6-V voltage source. 

□ 9 In Fig. 3-41, let circuit element X be a dependent current source with its 
arrow directed to the right and having a current of ij/3, where » 2 is the upward 
current through the 6-V source. Find i v 

□ 10 In Fig. 3-41, circuit element X is a dependent voltage source, 4tj/3, with 
the positive reference on the right side of the element. Let the power supplied 
by the 6-V source be 6f t ; find i v 

Dll In Fig. 3-42a, let S x , S 2 , and S 3 be 30-, 14-, and -2-V voltage sources, 
respectively, all with positive reference symbols on top. Use mesh analysis to 
find the power supplied by the 30-V source. 

i n 

Fig. 3-42 See Probs. 11 to 1 3 and 27. 

□ 12 In Fig. 3-42a, let S v S 2 , and S 3 be three current sources with currents of 
— 9, —1.5, and 6 A, respectively, flowing in an upward direction. Use mesh 
analysis to find the power supplied by the 6-A source. 

□ 13 Find the current i x in Fig. 3-42fc by: (a) nodal analysis; (b) mesh analysis; 
(c) changing the two practical voltage sources to practical current sources and 
then using nodal analysis; (d) changing the practical current source to a practical 
voltage source and again using nodal analysis. 

□ 1 4 (a) By beginning with the practical current source at the right in Fig. 3-43a, 
make repeated source transformations and resistance combinations in order to 
find the power supplied by the 24-V source, (b) What power does the 18-A source 

24 V 

18 A 




Fig. 3-43 See Probs. 14 to 16. 

□ 1 5 (a) Use superposition to determine the magnitude and direction of the current 
in the 4-J2 resistor of Fig. 3-43a. (b) How would the above result change if there 
were also a 40-V source, positive reference to the right, in series with the 4-fl 


1 03 $ ome Useful Techniques of Circuit Analysis 

D 1 6 Two current sources are connected to a resistive network as shown in Fig. 
3-43b. When the 3-A source is disconnected, it is found that the 2-A source 
delivers 28 W to the network and v 3 is 8 V. However, when the 2-A source is 
disconnected, the 3-A source supplies 54 W and v 2 is 12 V. Find the power 
supplied by each when both are operating. 

D 17 An automotive battery is found to be capable of supplying a load with 20 A 
at 12.3 V and 50 A at 12.0 V. (a) Represent the battery as a practical voltage 
source, (b) To what load resistance does the maximum power transfer theorem 
dictate a maximum load power is supplied? (c) What is the load power? (d) Under 
these conditions, what power would be dissipated within the battery? 

□ 1 8 Two terminals, a and b, extend from a black box containing an active resistive 
network. An ideal voltage source is connected across the terminals and it is found 
that when the voltage v ab is adjusted to 7.2 V no current flows from the source. 
Then an ideal current source is connected to the terminals, and it is found that 
v ab = when the current into the b terminal of the black box is 40 mA. Deter- 
mine the Thevenin and Norton equivalents of the black box. 

□ 1 9 Find the Thevenin and Norton equivalents of the circuits shown in: (a) Fig. 
3-44a; (b) Fig. 3-44b with R = oo; (c) Fig. 3-44b with R = 1.6 kfi. 


Fig. 3-44 See Prob. 1 9. 

D 20 For the two-terminal network shown in Fig. 3-45: (a) obtain a single equation 
relating v and i; (b) plot a curve of i versus v. 

Fig. 3-45 See Probs. 20 and 21 . 

1 04 Tha R»«i»Hve Circuit 

D 2 1 What is the maximum power that can be delivered to an external load resistor 
R L by the network of Fig. 3-45? 

□ 22 Two Thevenin equivalent circuits (c al and R v v, 2 and fl 2 ) are connected 
in parallel. Find the Thevenin equivalent of the resultant two-terminal network 
by using a method based on: (a) superposition; (b) source transformation. 

□ 23 Refer to the circuit shown in Fig. 3-35a and change the dependent voltage 
source 4v„ to a 2-W conductance. Draw a suitable tree and use general node 
voltages to determine v x and t)„. 

□ 24 Draw a suitable tree and analyze the circuit of Fig. 3-36a by using general 
node voltages to determine the power supplied by the 7-A source. 

□ 25 Draw an appropriate tree for the circuit of Fig. 3-35a, assign link currents, 
and use loop analysis to determine the power supplied by the dependent voltage 
source. (Note that the two control voltages can be expressed easily as currents 
and placed in links.) 

□ 26 Use loop analysis on the circuit shown in Fig. 3-46 to determine the magni- 
tude and direction of the current in the upper 2-fi resistor. 

20 V 

3 A 

Fig. 3-46 See Probs. 26 and 29. 

□ 27 Refer to the circuit shown in Fig. 3-42fc and decide whether general node 
or loop analysis will lead to the solution for i x most easily. Draw a suitable tree 
and find i r . 

D 28 Show that the network drawn in Fig. 3-47 is planar. 

D 29 After inspection of the network shown in Fig. 3-46, decide whether general 
node or loop analysis would be most expeditious in determining the current in 
the upper 2-0 resistor. Draw a suitable tree and find that current. 

D 30 Reconnect the common-base transistor amplifier of Fig. 3-38 in common- 
emitter configuration by interchanging r e and r b , by interchanging the labels 

Fig. 3-47 See Prob. 28. 

Emitter and Base, and by noting that i e is now directed vertically upward in the 
center leg. Find: (a) the ratio of the load voltage to the source voltage; (b) the 
ratio of the load current to the source current; (c) the ratio of the power delivered 
to the load to that supplied by the source. 











— — 


TKmTnrnillTIW rmflfflOl 

KffB^SP^ , *^» ■'■ : ■ "*'' '^' ' ' ' '' ''■ •firs; ^3Isr£ 


F fJISIffl 

110 The Transient Circuit 

elements. The independent and dependent voltage and current sources 
were called active elements and the linear resistor was termed a passive 
element, although our definitions of "active" and "passive" are still slightly 
fuzzy and need to be brought into sharper focus. We think of an active 
element as one which is capable of delivering net power to some external 
device, and the ideal sources were classified as such; a passive element, 
however, is capable only of receiving power and the resistor falls into this 
category. The energy it receives is usually transformed into heat. 

Each of these elements was defined in terms of the restrictions placed 
on its voltage-current relationship. In the case of the independent voltage 
source, for example, the terminal voltage must be completely independent 
of the current drawn from its terminals. We then considered circuits 
composed of the different building blocks. In general, we used only con- 
stant voltages and currents, but now that we have gained a familiarity with 
the basic analytical techniques by treating only the resistive circuit, we 
may begin to consider the much more interesting and practical circuits 
in which inductance and capacitance may be present and in which both 
the forcing functions and the responses usually vary with time. 


Both the inductor, which is the subject of this and the following section, 
and the capacitor, which is discussed later in the chapter, are passive 
elements which are capable of storing and delivering finite amounts of 
energy. Unlike an ideal source, they cannot provide an unlimited amount 
of energy or a finite average power. This concept may be used to improve 
upon our definition of an active element as being one which is capable 
of delivering an infinite amount of energy and of a passive element as one 
which is not capable of delivering infinite energy. 

Although we shall define an inductor and inductance strictly from a 
circuit point of view, that is, by a voltage-current equation, a few comments 
about the historic development of the magnetic field may provide a better 
understanding of the definition. In the early 1800s the Danish scientist 
Oersted showed that a current-carrying conductor produced a magnetic 
field, or that compass needles were affected in the presence of a cur- 
rent-carrying conductor. In France, shortly thereafter, Ampere made some 
careful measurements which demonstrated that this magnetic field was 
linearly related to the current which produced it. The next step occurred 
some twenty years later when the English experimentalist Michael Faraday 
and the American inventor Joseph Henry discovered almost simulta- 
neously 1 that a changing magnetic field could produce a voltage in a 

1 Faraday won. 


+ v - 

Fig. 4-1 The reference signs for voltage and current are shown on the circuit 
symbol for an inductor: v = L di/dt. 

neighboring circuit. They showed that this voltage was proportional to 
the time rate of change of the current which produced the magnetic field. 
The constant of proportionality we now call the inductance, symbolized 
by L, and therefore 

° = L i w 

where we must realize that v and i are both functions of time. When we 
wish to emphasize this, we may do so by using the symbols v(t) and i(t). 

The circuit symbol for the inductor is shown in Fig. 4-1, and it should 
be noted that the passive sign convention is used, just as it was with the 
resistor. The unit in which inductance is measured is the henry 2 (H), and 
the defining equation shows that the henry is just a shorter expression for 
a volt-second per ampere. 

The inductor whose inductance is defined by (1) is a mathematical 
model; it is an ideal element which we may use to approximate the behavior 
of a real device. A physical inductor may be constructed by winding a 
length of wire into a coil. This serves effectively to increase the current 
which is causing the magnetic field and also to increase the "number" of 
neighboring circuits into which Faraday's voltage may be induced. The 
result of this twofold effect is that the inductance of a coil is approximately 
proportional to the square of the number of complete turns made by the 
conductor out of which it is formed. An inductor, or "coil," which has 
the form of a long helix of very small pitch is found to have an inductance 
of fiN 2 A/s, where A is the cross-sectional area, s is the axial length of the 
helix, N is the number of complete turns of wire, and n (mu) is a constant 
of the material inside the helix, called the permeability. For air, ft = ju = 
4tt X 10- 7 H/m. 

Physical inductors should be on view in an accompanying laboratory 
course, and the topics concerned with the magnetic flux, permeability, and 
the methods of using the characteristics of the physical coil to calculate 
a suitable inductance for the mathematical model are treated in both 
physics courses and courses in electromagnetic field theory. 

Let us now scrutinize (1) to determine some of the electrical charac- 
teristics of this mathematical model. This equation shows that the voltage 
across an inductor is proportional to the time rate of change of the current 

2 An empty victory. 

112 Th* Transient Circuit 

through it. In particular, it shows that there is no voltage across an inductor 
carrying a constant current, regardless of the magnitude of this current. 
Accordingly, we may view an inductor as a "short circuit to dc." Another 
fact which is evidenced by this equation is related to an infinite rate of 
change of the inductor current, such as that caused by an abrupt change 
in current from one finite value to some other finite value. This sudden 
or discontinuous change in the current must be associated with an infinite 
voltage across the inductor. In other words, if we wish to produce an abrupt 
change in an inductor current, we must apply an infinite voltage. Although 
an infinite-voltage forcing function might be acceptable theoretically, it 
can never be a part of the phenomena displayed by a real physical device. 
As we shall see shortly, an abrupt change in the inductor current also 
requires an abrupt change in the energy stored in the inductor, and this 
sudden change in energy requires infinite power at that instant; infinite 
power is again not a part of the real physical world. In order to avoid 
infinite voltage and infinite power, an inductor current must not be allowed 
to jump instantaneously from one value to another. If an attempt is made 
to open-circuit a physical inductor through which a finite current is flowing, 
an arc may appear across the switch. The stored energy is dissipated in 
ionizing the air in the path of the arc. This is useful in the ignition system 
of an automobile, where the current through the spark coil is interrupted 
by the distributor, and the arc appears across the spark plug. 

We shall not consider any circuits at the present time in which an 
inductor is suddenly open-circuited. It should be pointed out, however, 
that we shall remove this restriction later when we hypothesize the exist- 

Rq. 4-2 (a) The current waveform in a 3-H inductor. {b\ The corresponding 
voltage waveform, v = 3 di/dt. 

t (s) 















V (V) 







t (s) 


1 1 3 Inductance and Capacitance 

ence of a voltage forcing function or response which does become infinite 

Equation (1) may also be interpreted (and solved, if necessary) by 
graphical methods. Let us assume a current which is zero prior to 
t = —Is, increases linearly to 1 A in the next second, remains at 1 A for 

2 s, and then decreases to zero in the next second, remaining zero there- 
after. The current waveform is sketched as a function of time in Fig. 4-2a. 
If this current is present in a 3-H inductor, and if the voltage and current 
senses are assigned to satisfy the passive sign convention, then we may use 
(1) to obtain the voltage waveform. Since the current is zero and constant 
for t < — 1, the voltage is zero in this interval. The current then begins 
to increase at the linear rate of 1 A/s, and thus a constant voltage of 3 V 
is produced. During the following 2-s interval, the current is constant and 
the voltage is therefore zero. The final decrease of the current causes a 
negative 3 V and no response thereafter. The voltage waveform is sketched 
in Fig. 4-2b on the same time scale. 

Let us now investigate the effect of a more rapid rise and decay of 
the current between the zero and 1-A values. If the intervals required for 
the rise and fall are decreased to 0.1 s, then the derivative must be ten 
times as great in magnitude. This condition is shown in the current and 
voltage sketches of Fig. 4-3a and b. In the voltage waveforms of Figs. 

Fig. 4-3 (a) The time required for the current of Fig. 4-2a to change from 
to 1 and from 1 to is decreased by a factor of 10. (b) The resultant 
voltage waveform. Note that the pulse widths are exaggerated slightly for 



i\ 3 






-1 / 


1_1 E 






12 3 




(to oo) 



2 3 
(to -oo) 


Fig. 4-4 (a) The time required for the current of Fig. 4-2a to change from 
to 1 and from 1 to is decreased to zero; the rise and fall are abrupt, 
(fc) The associated voltage across the 3-H inductor consists of a positive and 
negative infinite spike. 

4-2b and 4-3fc, it is interesting to note that the area under each voltage 
pulse is 3 V-s. 

A further decrease in the length of these two intervals will produce 
a proportionally larger voltage magnitude, but only within the interval in 
which the current is increasing or decreasing. An abrupt change in the 
current will cause the infinite voltage "spikes" (each having an area of 
3 V-s) that are suggested by the waveforms of Fig. 4-4a and b; or, from 
the equally valid but opposite point of view, these infinite voltage spikes 
are required to produce the abrupt changes in the current. It will be 
convenient later to provide such infinite voltages (and currents), and we 
shall then call them "impulses"; for the present, however, we shall stay 
closer to physical reality by not permitting infinite voltage, current, or 
power. An abrupt change in the inductor current is therefore temporarily 

Drill Problems 

4-1 For the circuit of Fig. 4-5o, find: (a) u t ; (b) u 2 ; (c) v 3 . 

Ans. -0.45; 0; 1.2 V 


0.8 H 

"3 (t)-0.8A 

Fig. 4-5 See Drill Probs. 4-1 and 4-2. 

4-2 The variation of current through a 20-mH inductor as a function of time 
is shown in Fig. 4-5b. Find the inductor voltage at t = : (a) 0.5; (b) 2.7; (c) 4.01 ms. 

Am. -0.3; 0.1; 0.2 V 


We have defined inductance by a simple differential equation 



and we have been able to draw several conclusions about the characteristics 
of an inductor from this relationship. For example, we have found that 
we may consider an inductor as a short circuit to direct current, and we 
have agreed that we cannot permit an inductor current to change abruptly 
from one value to another because this would require that an infinite voltage 
and power be associated with the inductor. The defining equation for an 
inductance still contains more information, however. Rewritten in a slightly 
different form, 

di = yvdt 


116 The Transiant Circuit 

it invites integration. Let us first consider the limits to be placed on the 
two integrals. We desire the current i at time t, and this pair of quantities 
therefore provides the upper limits on the integrals appearing on the left 
and right side of the equation, respectively; the lower limits may also be 
kept general by merely assuming that the current is i(t ) at time t . Thus 

I di =j- I vdt 

or i(t) - i(t ) = 7- f vdt 

and Kt) = ±f'vdt + i(t ) (3) 

Equation (2) expresses the inductor voltage in terms of the current, 
whereas (3) gives the current in terms of the voltage. Other forms are also 
possible for this latter equation. We may write the integral as an indefinite 
integral and include a constant of integration k, 

i(t) = ±-Cvdt+k (4) 

We may assume that we are solving a realistic problem in which the 
selection of t as - 00 ensures no current or energy in the inductor. Thus, 

if i(t ) = i(- 00) = 0, then 

i(t) = ±-fvdt (5) 

Let us consider the use of these several integrals by working a simple 
example. Suppose that the voltage across a 2-H inductor is known to be 
6 cos 5t V; what information is then available about the inductor current? 
From Eq. (3), 

i(t) = -i- J 6 cos 5* dt + i(t ) 


or i(t) = % % sin 5f - % % sin 5< + i(t ) = 0.6 sin 5t - 0.6 sin 5t + i(t ) 

The first term indicates that the inductor current varies sinusoidally; the 
second and third terms together merely represent a constant which becomes 
known when the current is numerically specified at some instant of time. 
Let us assume that the statement of our example problem also shows us 
that the current is 1 A at t = — zr/2 s. We thus identify * as -it/2, i(t ) 
as 1, and find that 

117 Inductance and Capacitance 

i(t) = 0.6 sin 5t - 0.6 sin (-2.5w) + 1 
or i(t) = 0.6 sin 5t + 1.6 

We may obtain the same result from (4). We have 

i(t) = 0.6 sin 5t + k 

and we establish the numerical value of k by forcing the current to be 
1 A at t = —w/2, 

1 = 0.6sin(-2.57r) + k 
or k = 1 + 0.6 = 1.6 

and i(t) = 0.6 sin 5t + 1.6 

once more. 

Equation (5) is going to cause trouble; it is based on the assumption 
that the current is zero when t = — oo. To be sure, this must be true in 
the real physical world, but we are working in the land of the mathematical 
model; our elements and forcing functions are all idealized. The difficulty 
arises after we integrate, 

I ' 
i(t) = 0.6 sin 5< 

and attempt to evaluate the integral at the lower limit, 

i(t) = 0.6 sin 5( - 0.6 sin ( - oo) 

The sine of ±oo is indeterminate; we might just as well represent it by 
an unknown constant, 

i(t) = 0.6 sin 5t + k 

and we see that this result is identical with that which we obtained when 
we assumed an arbitrary constant of integration in (4). 

We should not make any snap judgments, based on this example, as 
to which single form we are going to use forever; each has its advantages, 
depending on the problem and the application. Equation (3) represents 
a long, general method, but it shows clearly that the constant of integration 
is a current. Equation (4) is a somewhat more concise expression of (3), 
but the nature of the integration constant is suppressed. Finally, (5) is an 
excellent expression since no constant is necessary; however, it applies only 

118 The Transient Circuit 

when the current is zero at t = — oo and when the analytical expression 
for the current is not indeterminate there. 

Let us now turn our attention to power and energy. The absorbed 
power is given by the current-voltage product 

p = vi = U^- W 
r dt 

The energy w L accepted by the inductance is stored in the magnetic field 
around the coil and is expressed by the integral of the power over the 
desired time interval, 

f' pdt^Lf 1 i^-dt = L C i di = y 2 L{W)f - Wo)] 2 ) 

and thus 

«>i(*) - «>M = %MW*)] S - K'o)] 2 ) J ( 6 ) 

where we have again assumed that the current is i(t ) at time t . In using 
the energy expression, it is customary to assume that a value of t is selected 
at which the current is zero; it is also customary to assume that the energy 
is zero at this time. We then have simply 

w L (t) = y 2 L« 2 (7) 

where we now understand that our reference for zero energy is any time 
at which the inductor current is zero. At any subsequent time at which 
the current is zero, we also find no energy stored in the coil. Whenever 
the current is not zero, and regardless of its direction or sign, energy is 
stored in the inductance. It follows, therefore, that power must be delivered 
to the inductor for a part of the time and recovered from the inductor 
later. All the stored energy may be recovered from an ideal inductor; there 
are no storage charges or agent's commissions in the mathematical model. 
A physical coil, however, must be constructed out of real wire and thus 
will always have a resistance associated with it. Energy can no longer be 
stored and recovered without loss. 

These ideas may be illustrated by a simple example. In Fig. 4-6 an 
inductance of 3 H is shown in series with a resistance of 0.1 Q and a 
sinusoidal current source. The resistor may be interpreted, if we wish, as 
the resistance of the wire which must be associated with the physical coil. 

The voltage across the resistor is given by 

v„ = Ri = 1.2 sin ^-t 
R 6 

12sin?A( A. 

Fig. 4-6 A sinusoidal current is applied as a forcing function to a series 
RL circuit. 

and the voltage across the inductance is found by applying the defining 
equation for an inductance, 

v L = L^- = 3-i(l2 sin £ t \ = Oncost 
L dt dt\ 6 / 6 

The energy stored in the inductor is 

w L = %Li 2 = 216 sin 2 %t 

and it is apparent that this energy increases from zero at t = to 216 J 
at t = 3 s. During the next 3 s, the energy leaves the inductor completely. 
Let us see what price we have paid in this coil for the privilege of storing 
and removing 216 J in these few seconds. The power dissipated in the 
resistor is easily found as 


= i 2 R = 14.4 sin 2 ?-* 

and the energy converted into heat in the resistor within this 6-s interval 
is therefore 



p B dt = J 14.4 sin 2 — * 

c R = j 14.4(y 2 ) (l - cos jt\ dt = 43.2 J 

This represents 20 per cent of the maximum stored energy and is a reason- 
able value for many coils having this large an inductance. For coils having 
an inductance of about 100 jitH, we should expect a figure closer to 3 per 
cent. In Chap. 14 we shall formalize this concept by defining a quality 
factor Q that is proportional to the ratio of the maximum energy stored 
to the energy lost per period. 


1 20 T* 1 * Transient Circuit 

Let us now recapitulate by listing several characteristics of an inductor 
which result from its defining equation: 

1 There is no voltage across an inductor if the current through it is 
not changing with time. An inductance is therefore a short circuit 
to dc. 

2 A finite amount of energy can be stored in an inductor even if the 
voltage across the inductance is zero, such as when the current 
through it is constant. 

3 It is impossible to change the current through an inductor by a finite 
amount in zero time, for this requires an infinite voltage across the 
inductor. It will be advantageous later to hypothesize that such a 
voltage may be generated and applied to an inductor, but for the 
present we shall avoid such a forcing function or response. An 
inductor resists an abrupt change in the current through it in a 
manner analogous to the way a mass resists an abrupt change in 
its velocity. 

4 The inductor never dissipates energy, but only stores it. Although 
this is true for the mathematical model, it is not true for a physical 

Drill Problems 

4-3 Find the magnitude of the voltage across an inductor: (a) of 30 mH if the 
current through it is increasing at the rate of 20 mA/ms; (b) of 0.4 mH at t = 
if the current in it is 50e~ 10 *' mA; (c) at t = if the power entering it is given 
by 12 cos lOOwt mW and the inductor current is 150 mA at t = 0. 

Ans. 0.2; 0.08; 0.6 V 

4-4 Assuming the passive sign convention, find the current through a 0.1-H 
inductor at t = 2 s if : (a) v L == 0.5f V for < * < 3 s, v L = for * < and t > 3, 
andt L = 0att= -3;(b)v L = 0.5(t + 2) Vfor -2 < t < 1 s,v L = Ofort < -2 
and t > 1, and i t = at t = -3; (c) v L = 2/(t 2 + 4) V for all t, i t (- oo) = 0. 

Ans. 10.0; 22.5; 23.6 A 


Our next passive circuit element is the capacitor. We shall define capaci- 
tance C by the voltage-current relationship 

i = Cf (8) 

'» c 


Fig. 4-7 The current and voltage reference marks are shown on the circuit 
symbol for a capacitor so that i = C dv/dt. 

where v and t satisfy the conventions for a passive element, as shown in 
Fig. 4-7. From (8), we may determine the unit of capacitance as an 
ampere-second per volt, or coulomb per volt, but we shall now define the 
farad (F) as one coulomb per volt. 

The capacitor whose capacitance is defined by (8) is again a mathe- 
matical model of a real device. The construction of the physical device 
is suggested by the circuit symbol shown in Fig. 4-7, in much the same 
way as the helical symbol used for the inductor represents the coiled wire 
in that physical element. A capacitor, physically, consists of two conducting 
surfaces on which charge may be stored, separated by a thin insulating 
layer which has a very large resistance. If we assume that this resistance 
is sufficiently large that it may be considered infinite, then equal and 
opposite charges placed on the capacitor "plates" can never recombine, 
at least by any path within the element. Let us visualize some external 
device, such as a current source, connected to this capacitor and causing 
a positive current to flow into one plate of the capacitor and out of the 
other plate. Equal currents are entering and leaving the two terminals of 
the element, and this is no more than we expect for any circuit element. 
Now let us examine the interior of the capacitor. The positive current 
entering one plate represents positive charge moving toward that plate 
through its terminal lead; this charge cannot pass through the interior of 
the capacitor, and it therefore accumulates on the plate. As a matter of 
fact, the current and the increasing charge are related by the familiar 

l = ~dl 

Now let us pose ourselves a troublesome problem by considering this plate 
as an overgrown node and applying Kirchhoff 's current law. It apparently 
does not hold; current is approaching the plate from the external circuit, 
but it is not flowing out of the plate into the "internal circuit." This 
dilemma bothered a famous Scottish scientist about a century ago, and the 
unified electromagnetic theory which James Clerk Maxwell then developed 
hypothesizes a "displacement current" which is present wherever an 
electric field or voltage is varying with time. The displacement current 
flowing internally between the capacitor plates is exactly equal to the 
conduction current flowing in the capacitor leads; Kirchhoff 's current law 
is therefore satisfied if we include both conduction and displacement 


1 22 T* 1 ' Transient Circuit 

currents. However, circuit analysis is not concerned with this internal 
displacement current, and since it is fortunately equal to the conduction 
current, we may consider Maxwell's hypothesis as relating the conduction 
current to the changing voltage across the capacitor. The relationship is 
linear, and the constant of proportionality is obviously the capacitance C, 

•disp - « - C dt 

A capacitor constructed of two parallel conducting plates of area A, 
separated a distance d, has a capacitance C = eA/d, where e is the permit- 
tivity, a constant of the insulating material between the plates, and where 
the linear dimensions of the conducting plates are all very much greater 
than d. For air or vacuum, « = « = 8.854 pF/m = (l/367r) nF/m. 

The concepts of the electric field, displacement current, and the gener- 
alized form of Kirchhoff 's current law are more appropriate subjects for 
courses in physics and electromagnetic field theory, as is the determination 
of a suitable mathematical model to represent a specific physical capacitor. 

Several important characteristics of our new mathematical model can 
be discovered from the defining equation (8). A constant voltage across 
a capacitor requires zero current passing through it; a capacitor is thus 
an "open circuit to dc." This fact is certainly represented by the capacitor 
symbol. It is also apparent that a sudden jump in the voltage requires an 
infinite current. Just as we outlawed abrupt changes in inductor currents 
and the associated infinite voltages on physical grounds, we shall not permit 
abrupt changes in capacitor voltage; the infinite current (and infinite power) 
which results is nonphysical. We shall remove this restriction at the time 
we assume the existence of the current impulse. 

The capacitor voltage may be expressed in terms of the current by 
integrating (8). We first obtain 

dv = —i dt 

and then integrate between the times t and t and between the corre- 
sponding voltages v(t ) and v(t), 

1 r' 
v(t) = -J idt+v(t ) (9) 


Equation (9) may also be written as an indefinite integral plus a constant 
of integration, 

v(t) = -fidt + k (10) 

123 Inductance and Capacitance 

Finally, in many real problems, t may be selected as — oo and «(— oo) 
as zero, 


1 r* . 




Since the integral of the current over any time interval is the charge 
accumulated in that period on the capacitor plate into which the current 
is flowing, it is apparent that capacitance might have been defined as 

= Cv 

The similarity between the several integral equations introduced in this 
section and those appearing in our discussion of inductance is striking and 
suggests that the duality we observed between mesh and nodal equations 
in resistive networks may be extended to include inductance and capaci- 
tance as well. The principle of duality will be presented and discussed 
later in this chapter. 

As an illustration of the use of the several integral equations displayed 
above, let us find the capacitor voltage which is associated with thfe current 
shown graphically in Fig. 4-8a. We shall assume that the single 20 mA 
rectangular pulse of 2 ms duration is applied to a 5-fiF capacitor. Inter- 
preting (9) graphically, we know that the difference between the values 
of the voltage at t and t is proportional to the area under the current 
curve between these same two values of time. The proportionality constant 
is 1/C. The area can be obtained from Fig. 4-8a by inspection for desired 

Fig. 4-8 (a) The current waveform applied to a 5-/AF capacitor, [b) The 
resultant voltage waveform, easily obtained by integrating graphically. 



' ) ' 



! 3 

4 (ms) 




1 24 The Transient Circuit 

values of t and t. Thus, if 1 = -0.5 and * = 0.5 (in ms), 

u(0.5) = 2 + o(-0.5) 
or, if t = and t — 3, 

c(3) = 8 + v(0) 

We may express our results in more general terms by dividing the inter- 
esting range of time into several intervals. Let us select our starting point 
t prior to zero time. Then the first interval of t is selected between t 
and zero, 

V(t) = + V(t ) t < t < 

and since our waveform implies that no current has ever been applied to 
this capacitor since the Creation, 

v(t ) = 
and, thus, 

v(t) = t < 

If we now consider the time interval represented by the rectangular pulse, 
we obtain 

v(t) = 4000* < t < 2 ms 
For the semi-infinite interval following the pulse, we have 

v(t) = 8 t > 2 ms 

The results for these three intervals therefore provide us with analytical 
expressions for the capacitor voltage at any time after t = t ; the time t , 
however, may be selected as early as we wish. The results are expressed 
much more simply in a sketch than by these analytical expressions, as shown 
in Fig. 4-8b. 

The power delivered to a capacitor is 

p = t» = Cu#- 

r dt 

and the energy stored in its electric field is therefore 

/•' r' dv r* 

J pdt=Cj v-j-dt = Cj vdv = Y 2 C{[v(t)] 2 - [v(t )] 2 } 

to to Ul tHto) 

100 sin 2xt V 

Fig. 4-9 A sinusoidal voltage source is applied to a parallel RC network. 

and thus 

wM - WoCb) = V 2 C{[v(t)] 2 - [v(t )] 2 } 


where the stored energy is tt> c (* ) and the voltage is v(t ) at t . If we select 
a zero-energy reference at t , implying that the capacitor voltage is also 
zero at that instant, then 

wM = %Co* 


Let us consider a simple numerical example. As sketched in Fig. 4-9, 
we shall assume a sinusoidal voltage source in parallel with a 1-MQ resistor 
and a 20-juF capacitor. The parallel resistor may be assumed to represent 
the resistance of the insulator or dielectric between the capacitor plates. 
The current through the resistor is 

i H = £ = 10-" sin 2irt 

and the current through the capacitor is 

» r = C^f- = 20 X 10- 6 -f (100 sin 2irt) = 4w X 10~ 3 cos 2irt 
at at 

We next obtain the energy stored in the capacitor, 

w c = y 2 Ci> 2 = 0.1 sin 2 2-nt 

and see that the energy increases from zero at t = to a maximum of 0.1 J 
at t — % s and then decreases to zero in another % s. During this % s 
interval, the energy dissipated in the resistor is 

J- 0.5 ~0.5 

I p B dt — I 10- 2 sin 2 2irt dt = 2.5 mj 
n •'ft 

Thus, an energy equal to 2.5 per cent of the maximum stored energy is 
lost in the process of storing and removing the energy in the ideal capacitor. 


1 26 The Transient Circuit 

Much smaller values are possible in "low-loss" capacitors, but these smaller 
percentages are customarily associated with much smaller capacitors. 
Some of the important characteristics of a capacitor are now apparent: 

1 The current through a capacitor is zero if the voltage across it is 
not changing with time. A capacitor is therefore an open circuit 
to dc. 

2 A finite amount of energy can be stored in a capacitor even if the 
current through the capacitor is zero, such as when the voltage 
across it is constant. 

3 It is impossible to change the voltage across a capacitor by a finite 
amount in zero time, for this requires an infinite current through 
the capacitor. It will be advantageous later to hypothesize that such 
a current may be generated and applied to a capacitor, but for the 
present we shall avoid such a forcing function or response. A 
capacitor resists an abrupt change in the voltage across it in a 
manner analogous to the way a spring resists an abrupt change in 
its displacement. 

4 The capacitor never dissipates energy, but only stores it. Although 
this is true for the mathematical model, it is not true for a physical 

It is interesting to anticipate our discussion of duality by rereading the 
previous four statements with certain words replaced by their "duals." If 
capacitor and inductor, capacitance and inductance, voltage and current, 
across and through, open circuit and short circuit, spring and mass, and 
displacement and velocity are interchanged (in either direction), the four 
statements previously given for inductors are obtained. 

Drill Problems 

4-5 Find the current through a 0.01-jiF capacitor at t = if the voltage across 
it is: (a) 2 sin 2w 10 6 t V; (b) -2e- 10H V; (c) -2g- 107 ' sin 2w 10 6 f V. 

Ans. -0.1256; 0.1256; 0.2 A 

4-6 Find the voltage across a 0.01-ftF capacitor at t = 0.25 jus if v(0) = 0.6 V 
and the current through it is: (a) 0.2 sin 2w 10 6 ( A; (b) 0.2<r 107 ' A; (c) 0.2 A, 
< t < 2 jis. 

Ans. 2.44; 3.78; 5.60 V 

4-7 A 1000-pF capacitor, a 1-mH inductor, and a current source of 2 cos 10 6 t mA 
are in series. The capacitor voltage is zero at ( = 0. Find the energy stored: 

1 27 Inductance and Capacitance 

(a) in the inductor at t = 0; (b) in the capacitor at t = 1.571 fis; (c) in both inductor 
and capacitor together at t = 1 jus. 

Ans. 2; 2; 2 nj 


Now that we have added the inductor and capacitor to our list of passive 
circuit elements, we need to decide whether or not the methods we have 
developed in studying resistive circuit analysis are still valid. It will also 
be convenient to learn how to replace series and parallel combinations of 
either of these elements with simpler equivalents, just as we did with 
resistors in Chap. 2. 

We look first at Kirchhoff's two laws, both of which are axiomatic. 
However, when we hypothesized these two laws, we did so with no restric- 
tions as to the types of elements constituting the network. Both, therefore, 
continue to remain valid. 

Now we may extend the procedures we have derived for reducing 
various combinations of resistors into one equivalent resistor to the analo- 
gous cases of inductors and capacitors. We shall first consider an ideal 
voltage source applied to the series combination of N inductors, as shown 
in Fig. 4- 10a. We desire a single equivalent inductor L eq which may replace 
the series combination such that the source current i(t) is unchanged. The 
equivalent circuit is sketched in Fig. 4-10fo. For the original circuit 

v s = v 1 + v 2 + ■ ■ ■ + v N 

_ r di . T di , , T di 

- Ll Ji + L2 'dt + '"' +L "Tt 

= (L 1 + L 2 + ... +L N )f t 

or, written more concisely, 

W— l n~l n~l 

Fig. 4-10 (a) A circuit containing N inductors in series, (b) The desired 
equivalent circuit, in which L eq ~ L-l + L. 2 + ■ • ■ + L N , 


>N% L N c .( 


1 28 The Transient Circuit 

But for the equivalent circuit we have 

« - L 4L 

V '- L '"dt 

and thus the equivalent inductance is 


L eq = L l + L 2 + ■ ■ ■ + L N ° r L eq = 2 L » 


The inductance which is equivalent to several inductances connected in 
series is simply the sum of the series inductances. This is exactly the same 
result we obtained for resistors in series. 

The combination of a number of parallel inductors is accomplished by 
writing the single nodal equation for the original circuit, shown in Fig. 
4-1 la, 

*•= £'» = 2 \tJ •>* + <.('(>) 

n=l n=l LL n J t J 

r N 1 1 r< N 

L »=l ^n J J to n=l 

and comparing it with the result for the equivalent circuit of Fig. 4-11&, 

l r' 

Since Kirchhoff's current law demands that i s (t ) be equal to the sum of 
the branch currents at t , the two integral terms must also be equal; hence, 

L = 1 

"« ' l/L x + l/L 2 + ... +i/L N 

For the special case of two inductors in parallel, 

eq L x + L 2 

Fig. 4-1 1 (a) The parallel combination of N inductors, {b) The equivalent 
circuit, where L eq = 1/(1/Lj + 1/L 2 + ■ • • + 1/L N ). 

i • 1 

(a) (6) 

'W« C N V -(Z) 

(<•) (6) 

Fig. 4-12 (a) A circuit containing N capacitors in series, (b) The desired 
equivalent, C„ = 1/(1/0, + 1/G, + • • ■ + 1/C„). 

and we note that inductors in parallel combine exactly as do resistors in 

In order to find a capacitance which is equivalent to N capacitors in 
series, we use the circuit of Fig. 4- 12a and its equivalent Fig. 4-12b to 

f K r i .1 -i 

«. = 5>» = 2 Ur-J i<ft+»„(*o) 

»=1 n=lLC n ^ (0 J 


L n=l n JJ („ »=1 

1 /•' 

However, KirchhoflF's voltage law establishes the equality of v t (t ) and the 
sum of the capacitor voltages at t ; thus 

C — i 

" 1/Cj + 1/Cjj + • • • + 1/Cjy 

and capacitors in series combine as do resistors in parallel. 

Finally, the circuits of Fig. 4-13 enable us to establish the value of the 
capacitance which is equivalent to N parallel capacitors as 

C eq = C 1 + C 2 + ■■■ +C N 

Fig. 4-13 (a) The parallel combination of N capacitors, (b) The equivalent 
circuit, where C eq = C, + C 2 + ■ • • + C w . 


0.8 H 


1 jUF 

3 M F 


(o) (fe) 

Fig. 4-14 (a) A given LC network, (b) A simpler equivalent circuit. 

and it is no great source of amazement to note that capacitors in parallel 
combine in the same manner in which we combine resistors in series, that 
is, by simply adding all the individual capacitances. 

As an example in which some simplification may be achieved by com- 
bining like elements, consider the network of Fig. 4- 14a. The 6- and 3-juF 
capacitors are first combined into a 2-juF equivalent, and this capacitor 
is then combined with the 1-juF element with which it is in parallel to 
yield an equivalent capacitance of 3 juF. In addition, the 3- and 2-H 
inductors are replaced by an equivalent 1.2-H inductor which is then added 
to the 0.8-H element to give a total equivalent inductance of 2 H. The 
much simpler (and probably less expensive) equivalent network is shown 
in Fig. 4-l4b. 

The network shown in Fig. 4-15 contains three inductors and three 
capacitors, but no series or parallel combinations of either the inductors 
or the capacitors can be achieved. Simplification of this network cannot 
be accomplished at this time. 

Next let us turn to mesh, loop, and nodal analysis. Since we already 
know that we may safely apply Kirchhoff's laws, we should have little 
difficulty in writing a set of equations that are both sufficient and inde- 
pendent. They will be constant-coefficient linear integrodifferential equa- 
tions, however, which are hard enough to pronounce, let alone solve. 
Consequently, we shall write them now to gain familiarity with the use 
of Kirchhoff's laws in RLC circuits and discuss the solution of the simpler 
cases in the following chapters. 

Fig. 4-15 An LC network in which no series or parallel combinations of 
either the inductors or the capacitors ore possible. 




6 juF 


Fig. 4-16 A four node RLC circuit with node voltages assigned. 

Let us attempt to write nodal equations for the circuit of Fig. 4-16. 
Node voltages are chosen as indicated, and we sum currents leaving the 
central node, 

if ("i - ».) dt + *M + Vl R " 2 + c 2 

dv t 


where i L (t ) is the value of the inductor current at the time the integration 
begins, or the initial value. At the right node, 



i. = 

Rewriting these two equations, we have 

c, _ dv. If* , », i r' . , , , 
■R +C *-* + Ll v * dt -R=Ll v ' dt -^ 

v.. v 9 „ dv 9 dv. 

■r + r + c *-* =c >-* +1 - 

These are the promised integrodifferential equations, and we may note 
several interesting points about them. First, the source voltage t> s happens 
to enter the equations as an integral and as .a derivative, but not simply 
as v s . Since both sources are specified for all time, we should be able to 
evaluate the derivative or integral. Secondly, the initial value of the 
inductor current, i L (t ), acts as a (constant) source current at the center 

We shall not attempt the solution of these equations at this time. It 
is worthwhile pointing out, however, that when the two voltage forcing 
functions are sinusoidal functions of time it will be possible to define a 
voltage-current ratio (called impedance) or a current-voltage ratio (called 


I 32 The Transient Circuit 

admittance) for each of the three passive elements. The factors operating 
on the two node voltages in the equations above will then become simple 
multiplying factors, and the equations will be linear algebraic equations 
once again. These we may solve by determinants or a simple elimination 
of variables as before. 

Drill Problem 

4-8 In the circuit shown in Fig. 4-17, o x = 3e- 2xwn V. Find: (a) v 2 ; (b) v 3 ; 
(c) v.. 

Ans. -2.4e- 2xw "; 3.6e- 2x10 ''; 6e- 2xWH V 

15 mH 

500 Q ^-^ 40 mH 0.0S *tF 

AAA — (--y — <Tnnr> — 

0.12 juF 

Fiej. 4-17 See Drill Prob. 4-8. 


Duality has been mentioned earlier in connection with resistive circuits 
and more recently in the discussion of inductance and capacitance; the 
comments made were introductory and a little offhand. Now we may make 
an exact definition and then use the definition to recognize or construct 
dual circuits and thus avoid the labor of analyzing both a circuit and its 

We shall define duality in terms of the circuit equations. Two circuits 
are duals if the mesh equations that characterize one of them have the 
same mathematical form as the nodal equations that characterize the other. 
They are said to be exact duals if each mesh equation of the one circuit 
is numerically identical with the corresponding nodal equation of the other; 
the current and voltage variables themselves cannot be identical, of course. 
Duality itself merely refers to any of the properties exhibited by dual 

Let us interpret the definition and use it to construct an exact dual 
circuit by writing the two mesh equations for the circuit shown in Fig. 
4-18. Two mesh currents « x and » 2 are assigned, and the mesh equations 

3Q 8F 

:v(T) ^) B4H^») 


Fig. 4-18 A given circuit to which the definition of duality may be applied 
to determine the dual circuit. 

3i 1 + 4.^i-4^- = 2cos6t (14) 

dt dt 

-4 + 4 + iL(> t+5i 2=- 10 < 15 > 

It should be noted that the capacitor voltage v c is assumed to be 10 V 
at * = 0. 

We may now construct the two equations which are the mathematical 
exact duals of Eqs. (14) and (15). We wish them to be nodal equations, 
and we thus begin by replacing the mesh currents ij and i 2 by two node- 
to-reference voltages «! and t> 2 . We obtain 

3„ + 4^1 _ 4^ = 2 cos M (16) 

dt dt 

and we now seek the circuit represented by these two nodal equations. 

Let us first draw a line to represent the reference node, and then we 
may establish two nodes at which the positive references for v x and v 2 
are located. Equation (16) indicates that a current source 2 cos 6t is con- 
nected between node 1 and the reference node, oriented to provide a 
current entering node 1. This equation also shows that a 3-U conductance 
appears between node 1 and the reference node. Turning to (17), we first 
consider the nonmutual terms, or those terms which do not appear in (16), 
and they instruct us to connect an 8-H inductor and a 5-B conductance 
(in parallel) between node 2 and the reference. The two similar terms in 
(16) and (17) represent a 4-F capacitor present mutually at nodes 1 and 
2; the circuit is completed by connecting this capacitor between the two 
nodes. The constant term on the right side of (17) is the value of the 
inductor current at t = 0; thus, i L (0) = 10 A. The dual circuit is shown 
in Fig. 4-19; since the two sets of equations are numerically identical, the 
circuits are exact duals. 

Dual circuits may be obtained more readily than by the above method, 
for the equations need not be written. In order to construct the dual of 


2cos6tAVV / / \ 1 .550 

Fig. 4-19 The exact dual of the circuit of Fig. 4-18. 

a given circuit, we think of the circuit in terms of its mesh equations. With 
each mesh we must associate a nonreference node, and, in addition, we 
must supply the reference node. On a diagram of the given circuit we 
therefore place a node in the center of each mesh and supply the reference 
node as a line near the diagram or a loop enclosing the diagram. Each 
element which appears jointly in two meshes is a mutual element and gives 
rise to identical terms, except for sign, in the two corresponding mesh 
equations. It must be replaced by an element which supplies the dual term 
in the two corresponding nodal equations. This dual element must therefore 
be connected directly between the two nonreference nodes which are 
within the meshes in which the given mutual element appears. The nature 
of the dual element itself is easily determined; the mathematical form of 
the equations will be the same only if inductance is replaced by capacitance, 
capacitance by inductance, conductance by resistance, and resistance by 
conductance. Thus, the 4-H inductor which is common to meshes 1 and 
2 in the circuit of Fig. 4-18 appears as a 4-F capacitor connected directly 
between nodes 1 and 2 in the dual circuit. 

Elements which appear only in one mesh must have duals which appear 
between the corresponding node and the reference node. Referring again 
to Fig. 4-18, the voltage source 2 cos 6t V appears only in mesh 1; its dual 
is a current source 2 cos Qt A which is connected only to node 1 and the 
reference node. Since the voltage source is clockwise sensed, the current 
source must be into-the-nonreference-node-sensed. Finally, provision must 
be made for the dual of the initial voltage present across the 8-F capacitor 
in the given circuit. The equations have shown us that the dual of this 
initial voltage across the capacitor is an initial current through the inductor 
in the dual circuit; the numerical values are the same, and the correct sign 
of the initial current may be determined most readily by considering both 
the initial voltage in the given circuit and the initial current in the dual 
circuit as sources. Thus, if v c in the given circuit is treated as a source, 
it would appear as — t> c on the right side of the mesh equation; in the dual 
circuit, treating the current i L as a source would yield a term — i L on the 
right side of the nodal equation. Since each has the same sign when treated 
as a source, then, if v^O) = 10 V, t L (0) must be 10 A. 



2 cos 6( AO 

2 cos 

Fig. 4-20 The dual of the circuit of Fig. 4-1 8 is constructed directly from 
the circuit diagram. 

The circuit of Fig. 4-18 is repeated in Fig. 4-20, and its exact dual is 
constructed on the circuit diagram itself by merely drawing the dual of 
each given element between the two nodes which are centered in the two 
meshes which are common to the given element. A reference node which 
surrounds the given circuit may be helpful. After the dual circuit is redrawn 
in more standard form, it appears as shown in Fig. 4-19. 

An additional example of the construction of a dual circuit is shown 
in Fig. 4-21o and b. Since no particular element values are specified, these 
two circuits are duals, but not necessarily exact duals. The original circuit 
may be recovered from the dual by placing a node in the center of each 
of the five meshes of Fig. 4-21& and proceeding as before. 

The concept of duality may also be carried over into the language by 
which we describe circuit analysis or operation. One example of this was 
discussed previously in Sec. 4-4, and the duals of several words appeared 
there. Most of these pairs are obvious; whenever there is any question as 
to the dual of a word or phrase, the dual circuit may always be drawn 
or visualized and then described in similar language. For example, if we 
are given a voltage source in series with a capacitor, we might wish to 

Fig. 4-21 (a) The dual (in light lines) of a given circuit (in heavy lines) is 
constructed on the given circuit, (fc) The dual circuit is drawn in more con- 
ventional form. 




1 36 The Transient Circuit 

make the important statement, "the voltage source causes a current to flow 
through the capacitor"; the dual statement is, "the current source causes 
a voltage to exist across the inductor." The dual of a less carefully worded 
statement, such as, "the current goes round and round the series circuit," 
often requires a little inventiveness. 3 

Practice in using dual language can be obtained by reading Th6venin's 
theorem in this sense; Norton's theorem should result. 

We have spoken of dual elements, dual language, and dual circuits. 
What about a dual network? Consider a resistor R and an inductor L in 
series. The dual of this two-terminal network exists and is most readily 
obtained by connecting some ideal source to the given network. The dual 
circuit is then obtained as the dual source in parallel with a conductance 
G, G = R, and a capacitance C, C = L. We consider the dual network 
as the two-terminal network that is connected to the dual source; it is thus 
a pair of terminals between which G and C are connected in parallel. 

Before leaving the definition of duality, it should be pointed out that 
duality is defined on the basis of mesh and nodal equations. Since nonplanar 
circuits cannot be described by a system of mesh equations, a circuit which 
cannot be drawn in planar form does not possess a dual. 

We shall use duality principally to reduce the work which we must 
do to analyze the simple standard circuits. After we have analyzed the 
series RL circuit, then the parallel RC circuit requires less attention, not 
because it is less important, but because the analysis of the dual network 
is already known. Since the analysis of some complicated circuit is not 
apt to be well known, duality will usually not provide us with any quick 

Drill Problem 

4-9 Given this set of mesh equations: 

. di. If'., „ di„ 5 i* , „ dt, 1 r l 

- 2 ^-^i^ dt + 6 ^ + ef^ dt - 3 -di-2!j^ dt = 

1 r' ■ j 0*2 i r* . _, . n du 3r ( 

-- J ^ h dt-3-^--^ h dt + 4, 3 + 3-^ + -^ i 3 dt = 
consider the exact dual and let the numbering of the nodes correspond to the 
3 Someone has suggested, "the voltage is across all over the parallel circuit." 

1 37 Inducton** cmd Capacitance 

numbering of the mesh currents. Then, between what two nodes will there be 
found a: (a) current source? (b) 3-F capacitor? (c) 4-H inductor? 

Ans. 1, Ref.; 1,3; 2,3 


In the previous chapter we learned that the principle of superposition is 
a necessary consequence of the linear nature of the resistive circuits which 
we were analyzing. The resistive circuits are linear because the voltage- 
current relationship for the resistor is linear and Kirchhoff's laws are linear. 
We now wish to show that the benefits of linearity apply to RLC circuits 
as well. In accordance with our previous definition of a linear circuit, these 
circuits are also linear because the voltage-current relationships for the 
inductor and capacitor are linear relationships. For the inductor, we have 

r di 

v = L di 

and multiplication of the current by some constant K leads to a voltage 
which is also greater by a factor K. In the integral formulation, 

1 r' 

-J vdt + i L (t ) 

it can be seen that, if each term is to increase by a factor of K, then the 
initial value of the current must also increase by this same factor. That 
is, the factor K applies not only to the current and voltage at time t but 
also to their past values. 

A corresponding investigation of the capacitor shows that it too is 
linear. Thus, a circuit composed of independent sources, linear dependent 
sources, and linear resistors, inductors, and capacitors is a linear circuit. 

In this linear circuit the response is again proportional to the forcing 
function. The proof of this statement is accomplished by first writing a 
general system of integrodifferential equations, say, in terms of loop cur- 
rents. Let us place all the terms having the form of Ri, L di/dt, and 
(l/C)/i dt on the left side of each equation and keep the independent source 
voltages on the right side. As a simple example, one of the equations jnight 
have the form 

di 1 r' 
Ri + L-^ + -J i dt + o c («o) = v, 

If every independent source is now increased by a factor K, then the right 

1 38 The Transient Circuit 

side of each equation is greater by the factor K. Now each term on the 
left side is either a linear term involving some loop current or an initial 
capacitor voltage. In order to cause all the responses (loop currents) to 
increase by a factor K, it is apparent that we must also increase the initial 
capacitor voltages by a factor K. That is, we must treat the initial capacitor 
voltage as an independent source voltage and increase it also by a factor 
K. In a similar manner, initial inductor currents must be treated as inde- 
pendent source currents in nodal analysis. 

The principle of proportionality between source and response is thus 
extensible to the general RLC circuit, and it follows that the principle of 
superposition is also applicable. It should be emphasized that initial 
inductor currents and capacitor voltages must be treated as independent 
sources in applying the superposition principle; each initial value must take 
its turn in being rendered inactive. 

Before we can apply the superposition principle to RLC circuits, 
however, it is first necessary to develop methods of solving the equations 
describing these circuits when only one independent source is present. At 
this time we -should feel convinced that a linear circuit will possess a 
response whose amplitude is proportional to the amplitude of the source. 
We should be prepared to apply superposition later, considering an inductor 
current or capacitor voltage specified at t = t as a source which must be 
killed when its turn comes. 

Thevenin's and Norton's theorems are based on the linearity of the initial 
circuit, the applicability of Kirchhoff's laws, and the superposition princi- 
ple. The general RLC circuit conforms perfectly to these requirements, 
and it follows, therefore, that all linear circuits which contain any combi- 
nations of independent voltage and current sources, linear dependent 
voltage and current sources, and linear resistors, inductors, and capacitors 
may be analyzed with the use of these two theorems, if we wish. It is 
not necessary to repeat the theorems here, for they were previously stated 
in a manner that is equally applicable to the general RLC circuit. 


□ 1 A 2-H inductor is common to meshes 2 and 3 of a circuit. The mesh currents 
are: i 2 = 2e~°- 01t + 3 e -° 02t A and i 3 = -4e-°- 01 ' + 2e~°- 02 > A. At what value 
of t is the inductor voltage zero? 

□ 2 A current increases linearly from at t = to 0.4 A in 2 ms and decreases 
linearly from 0.4 A to in another 2 ms. The process repeats indefinitely, (a) 
Sketch the current, voltage, power, and energy for a 0.3-H inductor in the interval 
< t < 8 ms. (b) At what time is the power leaving the inductor exactly 10 W? 
(c) What energy is stored in the inductor at t = 6 ms? 

1 39 Inductance and Capacitance 

□ 3 Assume that 10 m of wire is available to construct a solenoid (an inductor 
in the form of a helix). Let the wire be lossless and of negligible diameter (for 
simplicity, not for accuracy). The cross section of the solenoid is circular and 
its length is three times its diameter. The medium is air. Find the dimensions 
and the number of turns if all the wire is used to make a 0.1-mH coil. 

□ 4 Given a voltage, v = 36 cos 200* V, across a 3-H inductor, find the inductor 
current at t = w/400 s if: (a) i t (0) = -0.1 A; (b) i L (-w/6Q0) = 0.02 A. 

□ 5 The voltage across a 20-juF capacitor is -2 V at t = -0.1 s and increases 
linearly at the rate of 50 V/s thereafter, (a) Sketch the capacitor current, voltage, 
power, and energy as functions of time, (b) Find the values of each of these 
quantities at ( = 0. 

□ 6 The current through a 4-juF capacitor is an infinite sequence of 100-mA pulses 
of 1-ms duration and 3-ms separation; that is, the period is 4 ms. The first pulse 
begins at t = when the capacitor has no voltage across it. (a) When does the 
capacitor voltage reach 1000 V? (b) What is the capacitor charge (in C) at 
t = 12 ms? (c) If the pulse amplitude is reduced to zero after t = 0.1 s, what 
is the energy stored in the capacitor at t = 0.2 s? 

□ 7 The voltage across a 10-nF capacitor is 6 V at t = and the current is 
12 sin 120ur mA. (a) What is the maximum capacitor voltage and when does it 
occur? (b) What is the maximum power drawn by the capacitor? 

D 8 Assume that air at standard temperature and pressure between two parallel 
conducting plates breaks down when the voltage across it is 30,000 V/cm of plate 
spacing. If each plate has an area of 0.01 m 2 and the separation is 1 mm, find: 

(a) C; (b) the maximum voltage possible across the capacitor; (c) the maximum 
energy that can be stored in this capacitor. 

□ 9 Given four nodes, A, B, C, and D, six 5-mH inductors are used to provide 
one inductor between each node pair. Find the equivalent inductance presented 
between nodes A and B, if the inductor is open-circuited that joins: (a) A to C; 

(b) C to D. 

□ 1 Given an inductor L v it is found that when a 1-H coil is placed in parallel 
with it and another 1-H coil is placed in series with this parallel combination, 
the equivalent inductance is still L t . (a) Find L v (b) Repeat if the 1-H coils 
are connected first in series and then in parallel. 

□ 1 1 Given a boxful of surplus 1-nF capacitors, how could you provide a: (a) 3.5-nF 
capacitance? (b) 3 / 4 -nF capacitance? 

D 12 All capacitance values are in juF for the network shown in Fig. 4-22. Find 
the equivalent capacitance offered at terminals: (a) b and e; (b) a and b. 

O 13 (a) Write a set of nodal integrodifferential equations for the circuit shown 




a "8 b 12 

Fig. 4-22 See Prob. 12. 

in Fig. 4-23a. Assume that the capacitor voltage ( + at top) and inductor current 
(arrow down) are known to be 0.6 V and 2.5 mA, respectively, at t = 0. (b) Repeat 
for loop or mesh equations. 

cos 10 4 « A 


-'TW V - 

Vq cos wt 


Fig. 4-23 See Probs. 1 3 to 15. 

□ 1 4 Write a set of loop or mesh integrodifferential equations for the circuit shown 
in Fig. 4-23b. Assume that the capacitor voltage ( + at left) and inductor current 
(arrow to right) are t> and i , respectively, at t = 0. (b) Repeat for nodal equations. 

□ 15 If the circuit shown in Fig. 4-236 is to be the exact dual of that in Fig. 4-23a, 
determine values (including units) for R, L, C, V , k, and the initial capacitor 
voltage ( + to right) and inductor current (arrow to right). 

□ 16 A voltage source, 10e -4 ' V, is connected to the series combination of 8 fi 
and 3 H. (a) Show that the circuit equations are satisfied by a current, 
i = — 2.5e -4 ' A. (b) Construct the exact dual of the above circuit, (c) Find the 
current through the capacitor in the dual circuit. 

□ 1 7 Determine the expressions for voltage division across two capacitors in series 
and for two inductors in series. Initial currents and voltages are assumed to be 


141 Inductance and Capacitance 

□ 1 8 Find formulas describing current division between two parallel capacitors 
and between two parallel inductors. Initial currents and voltages are assumed to 
be zero. 

□ 19 A capacitor C in series with a voltage source v a (t) is equivalent to the same 
capacitor C in parallel with a current source »,(*). (a) If »,(*) = 2 cos 10 6 t V and 
C = 10 4 pF, find i,(t). (b) Find »,(r) in terms of a general v,(t) and C. 

□ 20 The parallel combination of a current source i,(t) and an inductor L may 
be replaced by the series configuration of the inductor and a voltage source v,(t). 
Find v.(t) in terms of i,(t) and L. If L = 0.1 H and v, = i„ find c,. 

Source-free RL and 
RC Circuits 


hi the previous chapter we wrote equations governing tihe response of 
several circuits containing both inductance and capacitance, but we did 
not *ilw ;ui\ nf ihi-iii. Al this time we are reach/ to proceed with the 
solution for the simpler circuits. We shall restrict our attention to certain 
circuits which contain only resistors and inductors or only resistors and 
capacitors, and which contain no sources. We shall, however, allow the 
presence of energy which fe stored in the inductors or capacitors, for 
without such energy every response would be zero. 

143 Source-free KL and RC Circuits 

Although the circuits which we are about to consider have a very 
elementary appearance, they are also of practical importance. They find 
use as coupling networks in electronic amplifiers, as compensating networks 
in automatic control systems, as equalizing networks in communications 
channels, and in many other ways. A familiarity with these simple circuits 
will enable us to predict the accuracy with which the output of an amplifier 
can follow an input which is changing rapidly with time or to predict how 
quickly the speed of a motor will change in response to a change in its 
field current. Our knowledge of the performance of the simple RL and 
RC circuits will also enable us to suggest modifications to the amplifier 
or motor in order to obtain a more desirable response. 

The analysis of such circuits is dependent upon the formulation and 
solution of the integrodifferential equations which characterize the circuits. 
We shall call the special type of equation we obtain a homogeneous linear 
differential equation, which is simply a differential equation in which every 
term is of the first degree in the dependent variable and its derivatives. 
A solution is obtained when we have found an expression for the dependent 
variable, as a function of time, which satisfies the differential equation and 
also satisfies the prescribed energy distribution in the inductors or capacitors 
at a prescribed instant of time, usually t = 0. 

The solution of the differential equation represents a response of the 
circuit, and it is known by many names. Since this response depends upon 
the general "nature" of the circuit (the types of elements, their sizes, the 
interconnection of the elements), it is often called a natural response. It 
is also obvious that any real circuit we construct cannot store energy 
forever; the resistances necessarily associated with inductors and capacitors 
will eventually convert all stored energy into heat. The response must 
eventually die out, and it is therefore referred to as the transient response. 
Finally, we must also be familiar with the mathematician's contribution 
to the nomenclature; he calls the solution of a homogeneous linear differ- 
ential equation a complementary function. When we consider independent 
sources acting on a circuit, part of the response will partake of the nature 
of the particular source used; this part of the response will be "comple- 
mented" by the complementary response produced in the source-free 
circuit, and their sum will be the complete response. The source-free 
response may be called the natural response, the transient response, the 
free response, or the complementary function, but because of its more 
descriptive nature, we shall most often call it the natural response. 

We shall consider several different methods of solving these differential 
equations. This mathematics, however, is not circuit analysis. Our greatest 
interest lies in the solutions themselves, their meaning, and their inter- 
pretation, and we shall try to become sufficiently familiar with the form 
of the response that we are able to write down answers for new circuits 

1 44 The Transient Circuit 

by just plain thinking. Although complicated analytical methods are needed 
when simpler methods fail, an engineer must always remember that these 
complex techniques are only tools with which meaningful, informative 
answers may be obtained; they do not constitute engineering in themselves. 


We shall begin our study of transient analysis by considering the simple 
series RL circuit shown in Fig. 5-1. Let us designate the time- varying 
current as i(t), and we shall let the value of i(t) at t — be prescribed as 
I . We therefore have 

v B + v L = Ri + Lf t = 
f + fi = (1) 

and we must determine an expression for i(i) which satisfies this equation 
and also has the value I at t = 0. The solution may be obtained by several 
different methods. 

One very direct method of solving differential equations consists of 
writing the equation in such a way that the variables are separated and 
then integrating each side of the equation. The variables in (1) are i and 
t, and it is apparent that the equation may be multiplied by dt, divided 
by i, and arranged with the variables separated, 

f="f* ®> 

Since the current is I at t = and i(i) at time t, we may equate the two 
definite integrals which are obtained by integrating each side between the 
corresponding limits, 

r M ' -dt 

and, therefore, 

r m cU_ f'_R l 

, . I* R I 

In i = — — t \ 




L l 


i(t) = I e-« t/L (3) 


, + 




> V L 

+ ' 

Fig. 5-1 A series RL circuit for which «(*) is to be determined, subject to the 
initial condition that »(0} = I . 

We check our solution by first showing that substitution of (3) into (1) yields 
the identity = and then showing that substitution of t = into (3) 
produces i(0) = J . Both steps are necessary; the solution must satisfy the 
differential equation which characterizes the circuit, and it must also satisfy 
the initial condition, or the response at zero time. 

The solution may also be obtained by a slight variation of the method 
described above. After separating the variables, we may obtain the in- 
definite integral of each side of (2) if we also include a constant of integra- 
tion. Thus, 

and integration gives us 

\ni = - Z-t + K (4) 

The constant K cannot be evaluated by substitution of (4) into the original 
differential equation (1); the identity = will result, because (4) is a 
solution of (1) for any value of K. The constant of integration must be 
selected to satisfy the initial condition t(0) = I . Thus, at t = 0, (4) becomes 

and we use this value for K in (4) to obtain the desired response 
Ini = — yt + ln/ 

K*) = V" 


as before. 

Either of the methods above can be used when the variables can be 
separated, but this is only occasionally possible. In the remaining cases 

1 46 The Transient Circuit 

we shall rely on a very powerful method, the success of which will depend 
upon our intuition or experience. We shall simply guess or assume a form 
for the solution and then test our assumptions, first by substitution into 
the differential equation and then by applying the given initial conditions. 
Since we cannot be expected to guess the exact numerical expression for 
the solution, we shall assume a solution containing several unknown con- 
stants and select the values for these constants in order to satisfy the 
differential equation and the initial conditions. Many of the differential 
equations encountered in circuit analysis have a solution which may be 
represented by the exponential function or by the sum of several ex- 
ponential functions. Let us assume a solution of (1) in exponential form, 

i(t) = Ae 8 '' 

where A and s x are constants to be determined. After substituting this as- 
sumed solution into (1), we have 

A^e 8 '' + yAe*!' - 
or (s 1 + £)Ae s ' ( =0 

In order to satisfy this equation for all values of time, it is necessary that 
either A — 0, or s x = — oo, or s x = —R/L. But if A = or ^ = — oo, 
then every response is zero; neither can be a solution to our problem. 
Therefore, we must choose 


and our assumed solution takes on the form 

i(t) = Ae- Rl/L 

The remaining constant must be evaluated by applying the initial condition 
i — I at t — 0. Thus, 

and the final form of the assumed solution is 

i(t) = V*" (5) 

once again. 

147 Source-free Rl and RC Circuits 

We shall not consider any other methods for solving (1), although a 
number of other techniques may be used. Watch for them in a study of 
differential equations. 

Before we turn our attention to the interpretation of the response, let 
us check the power and energy relationships in this circuit. The power 
being dissipated in the resistor is 

Vr ■ 

i 2 R = I n 2 Re- 2Bt/L 

and the total energy turned into heat in the resistor is found by integrating 
the instantaneous power from zero time to infinite time, 

' R = f p R dt= I 2 R f e~ 2Rt ' L dt 
_ io K \ 2R) e | . ~ /2L1 ° 

This is the result we expect, because the total energy stored initially in 
the coil is y 2 W 2 > an< ^ there is no energy stored in the coil at infinite time. 
All the initial energy is accounted for by dissipation in the resistor. 

Drill Problems 

5-1 Each circuit shown in Fig. 5-2 has been in the condition shown for an 
extremely long time. At t = 0, the several switches are closed or opened as 
indicated. The single-pole double-throw switches appearing in b and c are drawn 
to indicate that they close one circuit before opening the other. They are called 
make before break. After reviewing the characteristics of an inductor, as sum- 
marized on page 120, determine i(0) in each circuit. 

Ans. -2; 2; 2.5 A 
Fig. 5-2 See Drill Probs. 5-1 , 5-2, and 5-5. 
t = 

i — w\ — -4--^- 

I en 
12 vi 

30 a 


8 H 


4 n 

148 ^* Transient Circuit 

5-2 At the instant just after the switches are thrown in the circuits of Fig. 5-2, 
find v. 

Ans. -10; -8; 20 V 

5-3 A 30-mH inductor is in series with a 400-S2 resistor. If the energy stored 
in the coil at t = is 0.96 /ij, find the magnitude of the current at t = : (a) 0; 
(b) 100 lis; (c) 300 /is. 

Ans. 0.147; 2.11; 8.00 mA 


Let us now consider the nature of the response in the series RL circuit. 
We found that the current is represented by 

i(t) = I Q e 


At zero time, the current is the assumed value I , and as time increases, 
the current decreases and approaches zero. The shape of this decaying 
exponential is seen by a plot of i(t)/I versus t, as shown in Fig. 5-3. Since 
the function we are plotting is e~ Rt/L , the curve will not change if R/L 
does not change. Thus, the same curve must be obtained for every series 
RL circuit having the same R/L or L/R ratio. Let us see how this ratio 
affects the shape of the curve. 

If we double the ratio of L to R, then the exponent will be unchanged 
if t is also doubled. In other words, the original response will occur at 
a later time, and the new curve is obtained by moving each point on the 
original curve twice as far to the right. With this larger L/R ratio, the 
current takes longer to decay to any given fraction of its original value. 
We might have a tendency to say that die "width" of the curve is doubled, 

Fig. 5-3 A plot of er u/L versus t. 

149 Source-free M and RC Circuits 

or that the "width" is proportional to L/R. However, we should have to 
define our term "width," because each curve extends from t — to oo. 
Instead, let us consider the time that would be required for the current 
to drop to zero if it continued to drop at its initial rate. 

The initial rate of decay is found by evaluating the derivative at zero 

— -i- = — — e - Rt / L — — B. 

Let us designate the value of time it takes for i// to drop from unity to 
zero, assuming a constant rate of decay, by the Greek letter t (tau). Thus, 

or t = | (7) 

The ratio L/R has the units of seconds since the exponent —Rt/L must 
be dimensionless. This value of time t is called the time constant; it is 
shown in Fig. 5-4. It is apparent that the time constant of a series RL 
circuit may easily be found graphically from the response curve; it is only 
necessary to draw the tangent to the curve at * = and determine the 
intercept of this tangent line with the time axis. 

An equally important interpretation of the time constant t is obtained 
by determining the value of i(t)/I at t = t. We have 

^1. = e- 1 = 0.368 or «(t) = 0.3687 

Fig. 5-4 The time constant t is L/R s for a series RL circuit. It is the time 
required for the response curve to drop to zero if it decays at a constant rate 
which is equal to its initial rate of decay. 


, , | 


T 2t 3r 

Fig. 5-5 The current in a series RL circuit is 36.8, 13.5, and 5 per cent of 
its initial value at T, 2t, and 3t, respectively. 

Thus, in one time constant the response has dropped to 36.8 per cent of 
its initial value; the value of t may also be determined graphically from 
this fact, as indicated by Fig. 5-5. It is convenient to measure the decay 
of the current at intervals of one time constant, and recourse to a slide 
rule or a table of negative exponentials shows that i{t)/l is 0.368 at ( = t, 
0.135 at t = 2t, 0.0498 at t = 3t, 0.0183 at t = 4t, and 0.0067 at t = 5t. 
At some point three to five time constants after zero time, most of us would 
agree that the current is a negligible fraction of its former self. 

Why does a larger value of the time constant L/R produce a response 
curve which decays more slowly? Let us consider the effect of each 
element. An increase in L allows a greater energy storage for the same 
initial current, and this larger energy requires a longer time to be dissipated 
in the resistor. We may also increase L/R by reducing R. In this case, 
the power flowing into the resistor is less for the same initial current; again, 
a greater time is required to dissipate the stored energy. 

In terms of the time constant t, the response of the series RL circuit 
may be written simply as 

i(t) = I e->" 

Drill Problem 

5-4 Find the inductance present in a series RL circuit if: (a) R is 40 £2 and the 
time constant is 30 ms; (b) the power dissipated in the 30-S2 resistor is cut in 
half every 20 ms; (c) the time constant is reduced from 16 to 15 ms by increasing 
the resistance 2 U. 

Ans. 0.48; 1.2; 1.73 H 


1 5 1 Source-free RL and RC Circuits 


It is not difficult to extend the results obtained for the series RL circuit 
to a circuit containing any number of resistors and one inductor. We 
fix our attention on the two terminals of the coil and determine the equiva- 
lent resistance across these terminals. The circuit is thus reduced to the 
simple series case. As an example, consider the circuit shown in Fig. 5-6. 
The equivalent resistance which the coil faces is 

R eq — fl 3 + fl 4 + 

fl l R 2 

Ri + fij 

and the time constant is therefore 

The inductor current t, is 


i L = «t(°) e 


and (8) represents what we might call the basic solution to the problem. 
It is quite possible that some current or voltage other than i L is needed, 
such as the current i 2 in R 2 . We can always apply Kirchhoff 's laws and 
Ohm's law to the resistive portion of the circuit without any difficulty, but 
current division provides the quickest answer in this circuit, 

R, +R, 

-i L (0)e~ 

It may also happen that we know the initial value of some current other 
than the inductor current. Since the current in a resistor may change 
instantaneously, we shall indicate the initial value after any change that 
might have occurred at t = by use of the symbol + ; in more mathe- 
matical language, i 1 (0 + ) is the limit from the right of i-^t) as t approaches 

Fig. 5-6 A source-free circuit containing one inductor and several resistors 
is analyzed by determining the time constant, t = L/R eq . 

1 52 Th * Transient Circuit 

zero. Thus, if we are given the initial value of t x as t 1 (0 + ), then it is apparent 
that the initial value of i 2 is 

From these values, we obtain the necessary initial value of i L (0) [or ^(O - ) 

or i L (0 + )], 

h/fi) = -[«!(0 + ) + i 2 (0 + )] = - Rl + R2 h(0 + ) 

and the expression for i 2 becomes 

h(° + )^e- 

Let us see if we can obtain this last expression more directly. Since 
the inductor current decays exponentially as e~ t/T , then every current 
throughout the circuit must follow the same functional behavior. This is 
made clear by considering the inductor current as a source current which 
is being applied to a resistive network. Every current and voltage in the 
resistive network must have the same time dependence. Using these ideas, 
we therefore express t 2 as 

t 2 = Ae~' /T 

and A must be determined from a knowledge of the initial value of i 2 . 
Since t^O" 1 ") is known, then the voltage across Rj and R 2 is known, and 

i 2 (0+) = i 1 (0 + )|i 


+ \^l-„-t/T 

A similar sequence of steps will provide a rapid solution to a large number 
of problems. We first recognize the time dependence of the response as 
an exponential decay, determine the appropriate time constant by com- 

Fig. 5-7 After t — 0, this circuit simplifies to an equivalent resistance of 
110 £2 in series with L eq = 2.2 mH. 

bining resistances, write the solution with an unknown amplitude, and then 
determine the amplitude from a given initial condition. 

This same technique is also applicable to a circuit which contains one 
resistor and any number of inductors, as well as to those special circuits 
containing two or more inductors and also two or more resistors that may 
be simplified by resistance or inductance combination until the simplified 
circuits have only one inductance or one resistance. As an example of such 
a circuit we may consider Fig. 5-7. After t = 0, when the voltage source 
is disconnected, we easily calculate an equivalent inductance, 

t = 2_X_3 + J _ 2.2 mH 
"> 2 + 3 

an equivalent resistance, 

"• 90 + 180 

and the time constant, 

L eq 2.2 x 10- 3 on 
T = —52- = = 20 us 

Re, HO 

Thus, the form of the natural response is Ae' 50 ' 000 *. With the independent 
source connected (t < 0), i L is 1 % , or 0.36 A, while i x is !%,,, or 0.2 A. 
At t — + , i L must still be 0.36 A, but i x will jump to a new value deter- 
mined by i L (0 + ). 

h(0 + ) = - i £ (0 + ) 18 %o = -0.24 A 



= 0.36 (t < 0) 

= O^e- 50 ' 000 ' (t > 0) 

1 54 The Transient Circuit 


i t = 0.2 (t < 0) 
= -0.24e- 50 - ooot 


In idealized circuits in which a pure inductance loop is present, such 
as that through the 2- and 3-mH coils of Fig. 5-7, a constant current may 
continue to circulate as t — > oo. The current through either of these 
inductors is not necessarily of the form, Ae~ t/T , but takes the more general 
form, A 1 + A 2 e~ t/T . This unimportant special case is illustrated by Prob. 
10 at the end of this chapter. 

We have now considered the task of finding the natural response of 
any circuit which can be represented by an equivalent inductance in series 
with an equivalent resistance. The most general RL circuit will be con- 
sidered in Sec. 5-7; the analysis is made more complicated because the 
response is composed of the sum of a number of negative exponentials. 

Drill Problems 

5-5 After t = 0, each of the circuits in Fig. 5-2 is source-free. Find expressions 

for i and v in each case for t > 0. 

Ans. 2.5e-° m A, - 10e-° st • V; 2e~ 2t A, -8e' 2 ' V; -2e" 5( A, 20e~ 5i V 

so n 

Fig. 5-8 See Drill Prob. 5-6 

5-6 For the circuit shown in Fig. 5-8, find: (a) i t (0+); (b) i L {10r 3 ); (c) ^(lO- 3 ). 

Ans. 54.1; 67.7; 500 mA 


The series combination of a resistor and a capacitor has a greater practical 
importance than does the combination of a resistor and an inductor. When 
an engineer has any freedom of choice between using a capacitor and using 
an inductor in the coupling network of an electronic amplifier, in the 
compensation networks of an automatic control system, or in the synthesis 

Fig. 5-9 A parallel RC circuit for which v(t) is to be determined, subject 
to the initial condition that u(0) = V . 

of an equalizing network, for example, he will choose the RC network over 
the RL network whenever possible. The reasons for this choice are the 
smaller losses present in a physical capacitor, its lower cost, the better 
approximation which the mathematical model makes to the physical ele- 
ment it is intended to represent, and the smaller size and lighter weight 
as exemplified by capacitors in hybrid and integrated circuits. 

Let us see how closely the analysis of the parallel (or is it series?) RC 
circuit corresponds to that of the RL circuit. The RC circuit is shown in 
Fig. 5-9. We shall assume an initial stored energy in the capacitor by 

o(0) = V 

The total current leaving the node at the top of the circuit diagram must 
be zero, and, therefore, 

Cf + | = 

Division by C gives us 

t + ife = ° < 9 > 

Equation (9) has a familiar form; comparison with (1), 

| + fi = (1) 

shows that the replacement of i by v and L/R by RC produces the identical 
equation we considered previously. It should, for the RC circuit we are 
now analyzing is the dual of the RL circuit we considered first. This duality 
forces v(t) for the RC circuit and i(t) for the RL circuit to have identical 
expressions if the resistance of one circuit is equal to the reciprocal of the 
resistance of the other circuit and if L is numerically equal to C. Thus, 


1 56 The Transient Circuit 

the response of the RL circuit, 

i(t) = i(0)e-* ,/L = l e- Rt/L 
enables us to write immediately 

v(t) = v(0)e-' /BC = V e-' /RC (10) 

for the RC circuit. 

Now let us suppose that we had selected the current i as our variable 
in the RC circuit, rather than the voltage v. Applying Kirchhoff 's voltage 

1 r* 

— I idt - v(t ) + Ri = 

we obtain an integral equation and not a differential equation. However, 
if we take the time derivative of both sides of this equation, 

and replace i by v/R, 

i + R f t = ° <"> 

RC^ dt 

we obtain (9) again. Equation (11) could have been used as our starting 
point, but duality would not have appeared as naturally. 

Let us discuss the physical nature of the voltage response of the RC 
circuit as expressed by (10). At t — we obtain the correct initial condi- 
tion, and as t becomes infinite the voltage approaches zero. This latter 
result agrees with our thinking that if there were any voltage remaining 
across the capacitor, then energy would continue to flow into the resistor 
and be dissipated as heat. Thus, a final voltage of zero is necessary. The 
time constant of the RC circuit may be found by using the duality rela- 
tionships on the expression for the time constant of the RL circuit, or it 
may be found by simply noting the time at which the response has dropped 
to 36.8 per cent of its initial value, 

and t = RC (12) 





0.368 V 

\ XJ 

\ j 

> t 

Fig. 5-10 The capacitor voltage v(t) in the parallel RC circuit is plotted as 
a function of time. The initial value of v(t) is assumed to be V . 

Our familiarity with the negative exponential and the significance of 
the time constant t enables us to sketch the response curve readily, Fig. 
5-10. Larger values of R or C provide a larger time constant and a slower 
dissipation of the stored energy. A larger resistance will dissipate a smaller 
power 1 with a given voltage across it, thus requiring a greater time to 
convert the stored energy into heat; a larger capacitance stores a larger 
energy with a given voltage across it, again requiring a greater time to 
lose this initial energy. 

Drill Problems 

5-7 For each of the circuits shown in Fig. 5-11, determine u(0 + ). 

Ans. 10; 50; 60 V 
Fig. 5-1 1 See Drill Probs. 5-7, 5-8, and 5-1 0. 

200 n 


t =0 

12 v -=- looo n< j_ + 


500 fi 90 V 



0.01 juF 

10 mA 



'"Greater resistance leads to less dissipation" might be the scholar's motto. 

1 58 ^ ne Transient Circuit 

5-8 For each of the circuits shown in Fig. 5-11, find «(0 + ). 

Ans. 6; 12.5; 20 mA 

5-9 A 2500-fi resistor is in series with a capacitor C. Find C if: (a) u c (0.1) = 
0.1 v c (0); (b) w c (0.1) = 0.05 w c (0); (c) u c (0) = 20 V and dv c /dt at t = is -400 

Ans. 17.4; 20.0; 26.7 fiF 


Many of the RC circuits for which we would like to find the natural response 
contain more than a single resistor and capacitor. Just as we did for the 
RL circuits, we shall first consider several special cases and save the general 
case for the final section in this chapter. 

Let us suppose first that we are faced with a circuit containing only 
one capacitor, but any number of resistors. It is possible to replace the 
two-terminal resistive network which is across the capacitor terminals by 
an equivalent resistance, and we may then write down the expression for 
the capacitor voltage immediately. For example, the circuit shown in Fig. 
5-12a may be simplified to that of Fig. 5-126, enabling us to write 


v = V e~ t/R "> c 

v(0) = V and R eQ = R 2 + 

R l fl 3 

R t + R 3 

Every current and voltage in the resistive portion of the network must have 
the form Ae~ t/Re " c , where A is the initial value of that current or voltage. 
Thus, the current in R v for example, may be expressed as 

Fig. 5-12 (a) A given circuit containing one capacitor and several resis- 
tors, [b) The resistors have been replaced by a single equivalent resistor; the 
time constant is now obvious. 


1 59 Source-free Rl and RC Circuits 


and i 1 (0 + ) remains to be determined from some initial condition. Suppose 
that u(0) is given. Since v cannot change instantaneously, we may think 
of the capacitor as being replaced by an independent dc source, «(0). Thus, 

i l( o +) - ..«2» *±- 

R 2 + fl^s/^j + R s ) R t + R 3 

The solution is obtained by collecting these results. 

Another special case includes those circuits containing one resistor and 
any number of capacitors. The resistor voltage is easily obtained by 
establishing the value of the equivalent capacitance and determining the 
time constant. Once again our mathematically perfect elements may lead 
to phenomena which would not exist in a physical circuit. Here, two 
capacitors in series may have equal and opposite voltages across each 
element and yet have zero voltage across the combination. Thus the general 
form of the voltage across either is A x + A 2 e~' /T , while the voltage across 
the series combination continues to be Ae~ t/T . An example of such a 
situation is provided by Prob. 20 at the end of the chapter. 

Some circuits containing a number of both resistors and capacitors may 
be replaced by an equivalent circuit containing only one resistor and one 
capacitor; it is necessary that the original circuit be one which can be 
broken into two parts, one containing all resistors and the other containing 
all capacitors, such that the two parts are connected by only two ideal 
conductors. This is not possible in general. 

Drill Problem 

5-10 Find v(t) and i(t) for t > for each of the circuits of Fig. 5-11. 

Ans. lOe- 10001 V, 20e- lom mA; SOe- 2 *-"** V, 
12.5e- a * 00t mA, 60e- 10t V, ftr 10 * mA 


A circuit containing several resistances and several inductances does not 
in general possess a form which allows either the resistances or inductances 
to be combined into single equivalent elements. There is no single negative 
exponential term or single time constant associated with the circuit. Rather, 

1 60 * ne Transient Circuit 

there will in general be several negative exponential terms, the number 
of terms being equal to the number of inductances which remain after all 
possible inductor combinations have been made. A similar condition holds 
for a general RC circuit, but for simplicity we shall restrict our attention 
to RL circuits. 

Let us visualize the problem which now confronts us. We have a circuit 
which must contain more than one loop, and hence a knowledge of several 
loop currents is required to describe the response. Each of these loop 
currents will be expressed as the sum of a number of negative exponentials, 
and each exponential will have an unknown amplitude and an unknown 
time constant. This represents a lot of unknown information. Our situation 
becomes somewhat more cheerful when we realize that each loop current 
should contain exponential terms with the same time constants as every 
other loop current. This appears plausible when we stop to consider that 
the voltages and currents throughout the circuit are related by a constant 
multiplier (resistors) or by differentiation or integration (inductors). Sums 
of these operations are also possible. Since none of these operations changes 
the exponent, we expect that each current or voltage must contain terms 
which may have every possible exponent. At any rate, we shall make this 
assumption; if we can satisfy the differential equations and the initial 
conditions, our assumption will be proved correct. 

Before we illustrate this method by an example, it must be realized 
that there are better and easier ways to find the natural response of these 
more complex circuits. One of the methods will appear toward the end 
of Chap. 13; it is based on the concept of complex frequency. The most 
powerful methods rely on the use of Fourier or Laplace transforms and 
will arise in Chaps. 18 and 19. 

Let us consider a specific circuit containing two inductors and two 
resistors, shown in Fig. 5-13. Mesh currents are assigned and the appro- 
priate set of mesh equations is written, 

, + 5§-3§ = (13) 

-4 + 4 +2i *=° (14) 

Fig. 5-13 An RL circuit having a response which must be described by the 
sum of two negative exponentials. 

i n 

161 Source-free RL and RC Circuits 

We shall assume that the initial values of i x and i 2 are known; let them 
be ^(0) and i 2 (0). We next assume an appropriate form for i x and t 2 and 
substitute the assumed expressions into the differential equations. We shall 
select a form for ij and i 2 which is the sum of two exponentials, 

»! = Ae"' + Be 82 ' (15) 

i 2 = Ce Sl ' + De 82 ' (16) 

and then substitute these expressions into the differential equations 

Ae 81 ' + Be 82 ' + 5As^' + 5Bs 2 e?*' - SC^e 8 '' - 3Ds 2 e?*' = 
-SA^e 81 ' - 3Bs^' + 3Cs^' + 3Ds 2 (? 2 ' + 2Ce 8 ' ( + 2De 82 ' = 

After factoring the exponentials, 

(A + 5A Sl - SCsjJe 8 '* + (B + 5Bs 2 - SOs^e 82 ' = 
(-3A*! + 3C Sl + 2C)e 8 »' + (-3Bs 2 + 3Ds 2 + 2D)e 82 ' = 

we realize that, in order that these expressions be zero for every value 
of t, each sum in parentheses must be zero. Hence, we obtain the four 

(5sj + 1)A - 3s t C = (17) 

(5s 2 + 1)B - 3s 2 D = (18) 

(3s 1 + 2)C - 3sjA = (19) 

(3« 2 + 2)D - 3s 2 B = (20) 

Eliminating A between (17) and (19), we have 

_3sjC__ (3» t + 2)C 
5*! + 1 ~~ 3sj 

or 6s x 2 + 13s! + 2 = 

and s 1 = — %, —2 

A similar manipulation of (18) and (20) yields 

s 2 = -y 6 , -2 

It makes no difference which answer is called s x and which is s 2 ; so we 
arbitrarily pick 

s 1 = — / 6 s 2 = — 2 

1 62 The Transient Circuit 


«! = Ae-' /6 + Be- 2 ' (21) 


i 2 = Ce- t/6 + De" 2( (22) 

The next step is the determination of A, B, C, and D. The given initial 
conditions must now be applied, 

VO) =A + B (23) 

i 2 (0) = C + D (24) 

These two equations are not sufficient to determine the four constants, 
and recourse must be had to (17) to (20). In other words, the differential 
equations impose certain restrictions among the amplitudes of the several 
current components. Let us select (17) and (18), 

(-% + 1)A + y 2 C = (-10+ 1)B + 6D = 
or A + 3C = (25) 

-9B + 6D = (26) 

The four equations (23) to (26) may be solved by eliminating variables or 
determinants. The results are easily obtained: 

A = 9 /u'i(0) - 6 /ui 2 (0) 
B = y^O) + e / n i 2 (0) 

c = - 3 AA(0) + 2 /h« 2 (0) 

D = 3/^,(0) + 9 / n « 2 (0) 

and the substitution of these results into (21) and (22) completes the mathe- 
matical solution. This circuit is analyzed by a much simpler method in 
Sec. 13-8 in accord with our comments earlier in this section. 

Let us select numerical values for the initial conditions and try to 
interpret the solution physically. Suppose we let tj(0) = 11 A and t 2 (0) = 
11 A. The initial current in the 3-H coil is, therefore, 

»i(0) - » 2 (0) = 11 - 11 = o 

although 11 A is flowing in the 2-H coil at t = 0. 
After evaluating the four amplitudes, we obtain 

ij = 3<r ,/6 + Se- 21 (27) 

i 2 = -e~' /6 + Vie-* (28) 

> ( <s) 

» t (?) 

Fig. 5-14 The current in (a) the 2-H coil and [b) the 3-H coil shown 
Fig. 5-13. 


i 1 — i 2 = 4e~' /6 — 4e~ 

The currents flowing in the two coils, % and i t — i 2 , are sketched in Fig. 
5- 14a and b by taking the difference or sum of the two exponential terms 
graphically. Energy is initially present in the 2-H coil, but its value drops 
quickly at first as some of the energy is transferred to the 3-H coil. This 
transfer is required because the initial voltage across the 2-S2 resistor is 22 V, 
and thus an initial rate of increase of current in the 3-H coil of 2 % A/s 
is established. Similarly, the current in the 2-H coil decreases initially at 
the rate of 15.5 A/s. Thus, energy is leaving the 2-H coil, some being 
transferred to the 3-H coil, but most being dissipated as heat in the two 

The two time constants, 6 s and 0.5 s, are not apparent in the circuit 
itself. Since they are quite unequal, however, we can at least identify the 
parts of the circuit which contribute to the longer and shorter time con- 
stant. For example, we may think of the circuit initially as being approxi- 


1 64 The Transient Circuit 

mately a 2-H coil in series with a 3-fi resistor. The 3-H coil is drawing 
a very small current; so we shall temporarily ignore it. The time constant 
of the early action is thus about 2/(1 + 2) or % s. At a much later time, 
the action slows down, a small rate of change of current is evident, and 
small voltages are present across both coils. Thus, a smaller voltage is across 
the 2-fl resistor. If we ignore it completely, the circuit acts as a 5-H coil 
in series with a 1-Q resistor. Thus the time constant is about 5 s. 

Drill Problems 

5-1 1 For the circuit of Fig. 5-15, for t > 0, find: (a) the smaller of the two time 
constants; (b) the larger of the two time constants; (c) the single time constant 
that would be present if the larger capacitor were replaced by a short circuit. 

Ans. 1; 1.2; 2 s 

t = 

18 V 

Fig. 5-15 See Drill Probs. 5-11 to 5-13. 

5-12 For the circuit of Fig. 5-15, find the value at t = 0+ of: (a) t^; (b) v 2 ; (c) 
v 3 . 

Ans. 2.25; 9; 9 V 

5-13 For the circuit of Fig. 5-15, for t > 0, determine: (a) v^t); (b) v 2 (t); (c) 

Ans. -2.25e- t + 4.5e~ t/2 V; 4.5e-' + 4.5<r i/2 V; 18 - 4.5e-' - 4.5e~' /2 V 


□ 1 For the circuit shown in Fig. 5-16, find i and v as functions of time for t > 0. 

Fig. 5-16 See Prob. 1. 

40 n t = o 
i — WV^Oj. 


v © 



10 mH 

1 65 Source-free ftt and RC Circuits 

D 2 A 200-fi resistor is in series with an inductor L. The initial value of the 
inductor current is 5 mA and its value 5 ms later is 3 mA. Find the time constant 
and the inductance. 

□ 3 Both switches in the circuit of Fig. 5-17 are closed at t = 0. Find i^t), i 2 (t), 
and i 3 (r) for t > 0. 

Fig. 5-17 See Prob. 3. 

□ 4 The initial inductor current in the network of Fig. 5-18 is 150 mA. Find v(t) 
for t > 0. 

at) 6 a 

Fig. 5-18 See Prob. 4. 

□ 5 Change the control on the dependent current source in Fig. 5-18 from 
to 0.5i. Let v(0 + ) be 2 V and find i(t) for t > 0. 

□ 6 The switch in the circuit of Fig. 5-19 is opened at t = after having been closed 
for a very long time, (a) What is the voltage v across the switch at t = + ? (b) 
Find v(t) for t > 0. 


Fig. 5-19 See Prob. 6. 

□ 7 A 1.5- V battery having an internal resistance of 0.5 Q is in series with a switch 
and an inductor L. In parallel with the inductor is a resistor R. Assume that 
the inductor is ideal. Select values for L and R such that the voltage across R 

1 66 The Transient Circuit 

jumps from zero to 1000 V as the switch is opened and does not drop below 100 V 
until 1 ms later. 

□ 8 Let the initial current in a source-free series RL circuit be I . Show that the 
total charge flowing through R between ( = and t = oo is the same as that 
which would flow if the current remained /„ for one time constant. 

□ 9 The left switch in the circuit of Fig. 5-20 is closed at t = 0. (a) Find i L (t) 
and i^t) for < t < 0.1 s. (b) The right switch is then closed at t = 0.1 s. Find 
i L (t) and i 1 (f) for t > 0.1 s. 

2 n 


4 Si 


24 V^ 

-f — <W\ — f — "W\ — I 

V,t~D K,t - 0.1 si 
-*\ "*A 3 0.6 H 



Fig. 5-20 See Prob. 9. 

□ 10 The two switches in the circuit of Fig. 5-21 are thrown simultaneously at 
* = 0. (a) Find ^(0+), i 2 (0 + ), and i(0 + ). (b) find L eq and t. (c) Write »(*) for t > 0. 
(d) To find i 1 (f) or i 2 (i), it is necessary to include a possible constant current present 
in the inductive loop. This may be done by finding the voltage across the 6-52 
resistor, which is the voltage across each coil, and integrating the inductor voltage 
to find the current; the known initial value is used as the constant of integration. 
Find i-^i) and i 2 (t). (e) Show that the sum of the energies remaining in the two 
coils as t —> oo plus that dissipated since t = in the resistor is equal to the sum 
of the inductor energies at ( = 0. 

Fig. 5-21 See Prob. 10. 

Dll After being closed for a long time, the switch in the circuit of Fig. 5-22 is 
opened at t = 0. Find v(i) for t > 0. 

Fig. 5-22 See Prob. 1 1 . 

0.3 V 


« «0 

A > s. 1 kfi J_+ ,,. 

t)0.6mA< 5 M F^ 

1 £7 Source-free RL and RC Circuits 

D 12 A certain precision 1-fiF capacitor has very high resistance material used 
between its conducting surfaces. The capacitor is charged to 1 V at t = and 
disconnected from the source. It is found that the voltage drops to 0.9 V in 
100 hr. Find the insulation resistance. 

□ 1 3 The independent source in the circuit of Fig. 5-23 is 140 V for t < and 
for t > 0. Find i{t) and v (i). 

70 fi 

0.02 uF 20 n 

Fig. 5-23 See Prob. 13. 

D 14 After having been closed for a long time, the switch in the network of Fig. 
5-24 is opened at t = 0. Find v c (t) for t > 0. 


' j ° 20 n 
f— -VA— | 


Fig. 5-24 See Prob. 14. 

□ 1 5 With reference to the circuit shown in Fig. 5-25, let u(0) = 9 V. Find i(t) 
for t > 0. 

50 nF^pvit) 

Fig. 5-25 See Prob. 1 5. 

□ 1 6 Replace the dependent voltage source in Fig. 5-25 with a dependent current 
source, arrow directed upward, with control of — Find v(t) and i(t) if 
o(0) = 9 V. 

□ 1 7 Two resistive wires, each 1 m long with a resistance of 10 fi/cm, are parallel 
and connected together at both ends with a perfect conductor. A 1000-pF 
capacitor is connected directly between the wires at some unspecified point, (a) 
What is the maximum possible time constant? (b) If t = 0.3 us, what is the 
distance from the capacitor to the nearer short circuit? 

168 "" Tramienl Circuit 

D 18 The initial capacitor voltages in the circuit of Fig. 5-26 are vJO) = 10 V, 
t> 2 (0) = 4 V. At what value of t is i = 0? 

R a . 5-26 See Prob. 18. 

Q 19 The switch in the circuit shown in Fig. 5-27 has been at a for a long time. 
At t = it is moved to b, and at t = 1 s it is moved to c. At what value of t 

is v = 1 V? 

ioo kn 

Fig. 5-27 See Prob. 19. 

□ 20 Five circuit elements, a 2-, a 3-, and a 6-juF capacitor, a 2-mA current source, 
and a 0.1-MSJ resistor, have been connected in parallel since a week ago last 
Tuesday. At t = 0, a frenzy of switching removes the current source from the 
circuit and connects the three capacitors in series with the resistor, such that 
the initial capacitor voltages are series aiding, (a) Find the voltage across the 
resistor as a function of time, (b) Find the current through the capacitors, (c) 
By integrating the current and using the known initial conditions, find the voltage 
across each capacitor as a function of time, (d) What is the voltage across each 
capacitor as t approaches infinity? 

D 21 After remaining open for a long time, the switch in the circuit of Fig. 5-28 
is closed at t = 0. At what time after t = is i(t) a maximum magnitude? 

Fig. 5-28 See Prob. 21. 

200 a 

1 69 Souree-fres Rl and KC Circuits 

□ 22 The switch in the circuit of Fig. 5-29 closes at t = 0. Find i x (t) and i 2 (t) 
for t > 0. 

3 6 H 12 H 

18A(f) 4.5 12 


Fig. 5-29 See Prob. 22. 
□ 23 For the circuit shown in Fig. 5-30, find v^t) and v 2 (t) for t > 0. 

50 fi\ 

Fig. 5-30 See Prob. 23. 

Chapter Six 

The Application of 

the Unit-step Forcing 



We have just spent a chapter's worth of our time studying the response 
of RL and AC circuits when no source or forcing function was present. 
We termed this response the natural response because its form depends 
only on the nature of the circuit. The reason that any response at all is 
obtained arises from the possibility of an initial energy storage within the 
inductive or capacitivc elements iii the circuit. In many of the examples 
and problems, we were confronted with circuits containing sources and 
switches; we were informed that certain switching operations were per- 
formed at f = in order to remove all the sources from the circuit, while 

]71 The Application of the Unit-step Forcing Function 

leaving known amounts of energy stored here and there. In other words, 
we have been solving problems in which energy sources are suddenly 
removed from the circuit; how we must consider that type of response which 
results when energy sources are suddenly applied to a circuit. 

We shall devote this chapter to a study of the response which occurs 
when the energy sources which are suddenly applied are dc sources. After 
we have studied sinusoidal and exponential sources, we may then consider 
the general problem of the sudden application of a more general source. 
Since every electrical device is intended to be energized at least once, and 
since most devices are turned on and off many times in the course of their 
lives, it should be evident that our study will be applicable to many 
practical cases. Even though we are now restricting ourselves to dc sources, 
there are still innumerable cases in which these simpler examples corre- 
spond to the operation of physical devices. For example, the first circuit 
we shall analyze may be considered to represent the build-up of the field 
current when a dc motor is started. The generation and use of the rectan- 
gular voltage pulses needed to represent a number or a command in a digital 
computer provide many examples in the field of electronic or transistor 
circuitry. Similar circuits are found in the synchronization and sweep 
circuits of television receivers, in communication systems using pulse 
modulation, and in radar systems, to name but a few examples. Further- 
more, an important part of the analysis of most servomechanisms is the 
determination of their responses to suddenly applied constant inputs. 


We have been speaking of the "sudden application" of an energy source, 
and by this phrase we imply its application in zero time. The operation 
of a switch in series with a battery is thus equivalent to a forcing function 
which is zero up to the instant that the switch is closed and is equal to 
the battery voltage thereafter. The forcing function has a break or discon- 
tinuity at the instant the switch is closed. Certain special forcing functions 
which are discontinuous or have discontinuous derivatives are called sin- 
gularity functions, the two most important of these singularity functions 
being the unit-step function and the unit-impulse function. The unit-step 
function is the subject of this chapter; the unit impulse is discussed in 
Chaps. 18 and 19. 

We define the unit-step function as a function which is zero for all values 
of its argument which are less than zero and which is unity for all positive 
values of its argument. If we let x be the argument and represent the 
unit-step function by u, then u(x) must be zero for all values of x less than 
zero, and it must be unity for all values of x greater than zero. At x = 0, 
u(x) changes abruptly from to 1. Its value at x = is not defined, but 


Fig. 6-1 The unit-step function u(x) is shown as a function of x. 

its value is known for all points arbitrarily close to * = 0. We often indicate 
this by writing «(0 _ ) = and u(0 + ) = 1. The concise mathematical defini- 
tion of the unit-step function is 


(0 x 
ll x 


and it is shown graphically in Fig. 6-1. 

In order to obtain a unit-step forcing function, we must express the 
unit step as a function of time, and the simplest expression is obtained by 
replacing * by t, 



However, we cannot always arrange the operation of a circuit so that 
every discontinuity occurs at t — 0. If two switches are to be thrown in 
sequence, for example, we might elect to operate one of them at t = 0, 
and it is then necessary to throw the second switch at some later time 
t = t . Since the unit-step function provides us with a suitable discontinuity 
when the value of its argument is zero, then the operation of the second 
switch may be represented by selecting a unit-step forcing function having 
an argument (t — t ). Thus, 

u(t ■ 

f t < t„ 


This function is shown in Fig. 6-2. 

Fig. 6-2 The unit-step forcing function, u(t — t ). 


-> i 

Vu(t - t a )[ 




(a) (b) 

Fig. 6-3 (a) A voltage-step forcing function is shown as the source of a 
general network, [b) A simple circuit which, although not the exact equiva- 
lent of (a), may be used as its equivalent in many cases, (c) An exact 
equivalent of (a}. 

The unit-step forcing function is in itself dimensionless. If we wish it 
to represent a voltage, it is necessary to multiply u(t — t ) by some constant 
voltage, such as V. Thus, v(t) — Vu(t - t ) is an ideal voltage source which 
is zero before t = t and a constant V after t = t . This forcing function 
is shown connected to a general network in Fig. 6-3a. We should now 
logically ask what physical source is the equivalent of this discontinuous 
forcing function. By equivalent, we mean simply that the voltage-current 
characteristics of the two networks are identical. For the step-voltage 
source of Fig. 6-3a, the voltage-current characteristic is quite simple; the 
voltage is zero prior to t = t , it is V after t = t , and the current may 
be any (finite) value in either time interval. Our first thoughts might 
produce the attempt at an equivalent shown in Fig. 6-3fc, a dc source V 
in series with a switch which closes at t = t . This network is not equivalent 
for t < t , however, because the voltage across the battery and switch is 
completely unspecified in this time interval. The "equivalent" source is 
an open circuit, and the voltage across it may be anything. After t — t , 
the networks are equivalent, and if this is the only time interval in which 
we are interested, and if the initial currents which flow from the two 
networks are identical at t = t , then Fig. 6-3fo becomes a useful equivalent 
of Fig. 6-3a. 

In order to obtain an exact equivalent for the voltage-step forcing 
function, we may provide a single-pole double-throw switch. Before t = t , 
the switch serves to ensure zero voltage across the input terminals of the 
general network. After t = t , the switch is thrown to provide a constant 
input voltage V. At t = t , the voltage is indeterminate (as is the step 
function), the battery is momentarily short-circuited, and it is fortunate 
that we are dealing with mathematical models. This exact equivalent of 
Fig. 6-3a is shown in Fig. 6-3c. 

Before concluding our discussion of equivalence, it is enlightening to 
consider the exact equivalent of a battery and a switch. What is the 
voltage-step forcing function which is equivalent to Fig. 6-3b? We are 
searching for some arrangement which changes suddenly from an open 
circuit to a constant voltage; a change in resistance is involved, and this 






(a) (b) 

Fig. 6-4 (a) A current-step forcing function is applied to a general net- 
work, (b) A simple circuit which, although not the exact equivalent of (a), 
may be used as its equivalent in many cases. 

is the crux of our difficulty. The step function enables us to change a voltage 
discontinuously (or a current), but here we need a changing resistance as 
well. The equivalent therefore must contain a resistance or conductance 
step function, a passive element which is time-varying. Although we might 
construct such an element with the unit-step function, it should be apparent 
that the end product is a switch; a switch is merely a resistance which 
changes instantaneously from zero to infinite ohms, or vice versa. Thus, 
we conclude that the exact equivalent of a battery and switch in series 
must be a battery in series with some representation of a time-varying 
resistance; no arrangement of voltage- and current-step forcing functions 
is able to provide us with the exact equivalent. 1 

Figure 6-4a shows a current-step forcing function driving a general 
network. If we attempt to replace this circuit by a dc source in parallel 
with a switch (which opens at t = t ), we must realize that the circuits 
are equivalent after t = t , but the responses are alike after t — t only 
if the initial conditions are the same. Judiciously, then, we may often use 
the circuits of Fig. 6-4a and b interchangeably. The exact equivalent of 
Fig. 6-4a is the dual of the circuit of Fig. 6-3c; the exact equivalent of 
Fig. 6-4b cannot be constructed with current- and voltage-step forcing 
functions alone. 2 

Some very useful forcing functions may be obtained by manipulating 
the unit-step forcing function. Let us define a rectangular voltage pulse 
by the following conditions: 

The pulse is drawn in Fig- 6-5. Can this pulse be represented in terms 
of the unit-step forcing function? Let us consider the difference of the 

1 An equivalent may always be determined if some information about the general network 
is available (the voltage across the switch for t < t ); we assume no a priori knowledge about 
the general network. 
2 The equivalent can be drawn if the current through the switch prior to t = t is known. 



Fig. 6-5 A useful forcing function, the rectangular voltage pulse. 

two unit steps u(t — t ) — u(t — f x ). The two step functions are shown in 
Fig. 6-6a, and their difference is obviously a rectangular pulse. The source 
Vu(t — t ) — Vu(t — <j) which will provide us with the desired voltage is 
indicated in Fig. 6-6b. 


« (' - «o ) 

Vu(t-t )rf) 

Vu« - li)(lj 


-u(t - (,) 

<<■) (h) 

Fig. 6-6 (a) The unit steps u[t — t ) and — u{t — tj. (b) A source which 
yields the rectangular voltage pulse of Fig. 6-5. 

If we have a sinusoidal voltage source V sin cot which is suddenly 
connected to a network at t — t , then an appropriate voltage forcing 
function would be v(t) — Vu(t — t ) sin tot If we wish to represent one 
burst of energy from a radar transmitter, we may turn the sinusoidal source 
off y i0 /us later by a second unit-step forcing function. The voltage pulse 
is thus 

v(t) = V[u(t - t ) - u(t - t - 10" 7 )] sin ut 

This forcing function is sketched in Fig. 6-7. 

As a final introductory remark, we should note that the unit-step forcing 
function must be considered only as the mathematical model of an actual 
switching operation. No physical resistor, inductor, or capacitor behaves 
entirely like its idealized circuit element; we also cannot perform a switch- 
ing operation in zero time. However, switching times less than 1 ns are 
common in many circuits, and this time is often sufficiently short compared 
with the time constants in the rest of the circuit that it may be ignored. 



«o + 10 ~ 7 

Hg. 6-7 A radio-frequency pulse, described by v{t) = V[u(t — t ) — 
u[t — t — ^0~ 7 )] sin at. The sinusoidal frequency within the pulse shown 
is about 36 MHz, a value which is too low for radar, but about right for 
constructing legible drawings. 

Drill Problems 

6-1 With reference to the circuit shown in Fig. 6-8, express the following 
currents in step-function notation: (a) i^it); (b) i 2 (t); (c) i 3 (t). 

Am. 2 - 2.8u(t) - 0.2u(t - 1); 2 + 1.2u(t) - 0.2u(t - I); 
2 + 1.2u{t) + 0.2u(t - 1) A 

4u«) A 

Fig. 6-8 See Drill Prob. 6-1 . 

6-2 The voltage waveform, v(i) = 12«(t) - 16u(t - 3) V, is applied to a 2-H 
inductor. Using the passive sign convention, find the inductor current at * = : 

(a) 0; (b) 2; (c) 4 s. 

Ans. 0; 12; 16 A 


We are now ready to subject a simple network to the sudden application 
of a dc source. The circuit consists of a battery V in series with a switch, 
a resistance R, and an inductance L. The switch is closed at t = 0, as 
indicated on the circuit diagram of Fig. 6-9a. It is evident that the current 
i(r) is zero before t = 0, and we are therefore able to replace the battery 







Fig. 6-9 (a) The given circuit, [b) An equivalent circuit, possessing the 
same response <(*) for all time. 

and switch by a voltage-step forcing function Vu(t), which also produces 
no response prior to t = 0. After t = 0, the two circuits are obviously 
identical. Hence, we seek the current i(£) either in the given circuit of 
Fig. 6-9a or in the equivalent circuit of Fig. 6-9£>. 

We shall find »(f) at this time by writing the appropriate circuit equation 
and then solving it by separation of the variables and integration. After 
we obtain the answer and investigate the two parts of which it is composed, 
we shall next spend some time (the following section) in learning the general 
significance of these two terms. We can then construct the solution to this 
problem very easily; moreover, we shall be able to apply the general 
principles behind this simpler method to produce more rapid and more 
meaningful solutions to every problem involving the sudden application 
of any source. Let us now proceed with the more formal method of 

Applying Kirchhoff 's voltage law to the circuit of Fig. 6-9fc, we have 

Ri + L^- = Vu(t) 

Since the unit-step function is discontinuous at t = 0, we shall first consider 
the solution for t < and then for t > 0. It is evident that the application 
of zero voltage since t = — co has not produced any response, and, there- 

i(t) = ( < 
For positive time, however, u(t) is unity and we must solve the equation 

Ri + L^- = V 


The variables may be separated in several s 4 mple algebraic steps, yielding 




V- Ri 

= dt 

1 78 The Transient Circuit 

and each side may be integrated directly, 

4 In (V- Ri) = t + k 

In order to evaluate k, an initial condition must be invoked. Prior to t = 0, 
i(t) is zero, and thus t(0~) = 0; since the current in an inductor cannot 
change by a finite amount in zero time without being associated with an 
infinite voltage, we thus have i(0 + ) = 0. Setting i = at t — 0, we obtain 

and, hence, 


fmv = * 

■^[ln(V - Ri) -InV] = t 

V — Ri _ e -m/L 

i = ¥■ - v e - Rt/L t > 

R R 

Thus, an expression for the response valid for all t would be 

i = (|-| e - R(/t )«W (1) 

This is the desired solution, but it has not been obtained in the simplest 
manner. In order to establish a more direct procedure, let us try to interpret 
the two terms appearing in (1). The exponential term has the functional 
form of the natural response of the RL circuit; it is a negative exponential, 
it approaches zero as time increases, and it is characterized by the time 
constant L/R. The functional form of this part of the response is thus 
identical with that which is obtained in the source-free circuit. However, 
the amplitude of this exponential term depends on V. We might generalize, 
then, that the response will be the sum of two terms, where one term has 
a functional form which is identical with that of the source-free response, 
but has an amplitude which depends on the forcing function. Now let us 
consider the nature of the second part of the response. 

Equation (1) also contains a constant term V/R. Why is it present? 
The answer is simple: the natural response approaches zero as the energy 
is gradually dissipated, but the total response must not approach zero. 
Eventually the circuit behaves as a resistor and inductor in series with a 
battery, and a direct current V/R flows. This current is a part of the 

1 79 The Application of Hie Unit-step Forcing Function 

response which is directly attributable to the forcing function, and we call 
it the forced response. It is the response which is present a long time after 
the "switch is closed. 

The complete response is composed of two parts, the natural response 
and the forced response. The natural response is a characteristic of the 
circuit and not of the sources. Its form may be found by considering the 
source-free circuit, and it has an amplitude which depends on the initial 
amplitude of the source and the initial energy storage. The forced response 
has the characteristics of the forcing function; it is found by pretending 
that all switches have been thrown a long time ago. Since we are presently 
concerned only with switches and dc sources, the forced response is merely 
the solution of a simple dc circuit problem. 

The reason for the two responses, forced and natural, may also be seen 
from physical arguments. We know that our circuit will eventually assume 
the forced response. However, at the instant the switches are thrown, the 
initial currents in the coils (or the voltages across the capacitors in other 
circuits) will have values which depend only on the energy stored in these 
elements. These currents or voltages cannot be expected to be the same 
as the currents and voltages demanded by the forced response. Hence, there 
must be a transient period during which the currents and voltages change 
from their given initial values to their required final values. The portion 
of the response which provides the transition from initial to final values 
is the natural response (often called the transient response, as we found 
earlier). If we describe the response of the source- free simple RL circuit 
in these terms, then we should say that the forced response is zero and 
that the natural response serves to connect the initial response produced 
by stored energy with the zero value of the forced response. This descrip- 
tion is appropriate only for those circuits in which the natural response 
eventually dies out. This always occurs in physical circuits where some 
resistance is associated with every element, but there are a number of 
pathologic circuits in which the natural response is nonvanishing as time 
becomes infinite; those circuits in which trapped currents circulate around 
inductive loops or voltages are trapped in series strings of capacitors are 

Now let us search out the mathematical basis for dividing the response 
into a natural response and a forced response. 

Drill Problem 

6-3 A current source of 0.2u(t) A, a 100-S2 resistor, and a 0.4-H inductor are 
in parallel. Find the magnitude of the inductor current: (a) as t — * oo; (b) at 
t = + ; (c) at t = 4 ms. 

Ans. 0; 0.126; 0.200 A 

180 Th* Transiwil arcuit 


There is also an excellent mathematical reason for considering the complete 
response to be composed of two parts, the forced response and the natural 
response. The reason is based on the fact that the solution of any linear 
differential equation may be expressed as the sum of two parts, the com- 
plementary solution (natural response) and the particular solution (forced 
response). Without delving into the general theory of differential equations, 
let us consider a general equation of the type met in the previous section, 

^- + Pi = Q (2) 


We may identify Q as a forcing function and express it as Q(t) to emphasize 
its general time dependence. In all our circuits, P will be a positive 
constant, but the remarks that follow about the solution of (2) are equally 
valid for the cases in which P is a general function of time. Let us simplify 
the discussion by assuming that P is a positive constant. Later, we shall 
also assume that Q is constant, thus restricting ourselves to dc forcing 

In any standard text on elementary differential equations, it is shown 
that if both sides of this equation are multiplied by a so-called integrating 
factor, then each side becomes an exact differential which can be integrated 
directly to obtain the solution. We are not separating the variables, but 
merely arranging them in such a way that integration is possible. For this 
equation, the integrating factor is e SPdt or e™, since P is a constant. We 
multiply each side of the equation by this integrating factor and obtain 


The form of the left side may now be improved when it is recognized as 
the exact derivative of ie p ', 

dt dt 

and, thus, 

f t (ie") = Qe» 

We may now integrate each side with respect to time, finding 

fe pt = fQtf'dt + A 

181 Tto Application of the Unlt-«tep Forcing Function 

where A is a constant of integration. Since this constant is explicitly shown, 
we should remember that no integration constant needs to be added to 
the remaining integral when it is evaluated. Multiplication by e~ pi produces 
the solution for i(r), 

i = «-« J" Qj-t dt + Ae- p ' (3) 

If Q(t), the forcing function, is known, then it remains only to evaluate 
the integral to obtain the exact functional form for i(t). We shall not 
evaluate such an integral for each problem, however; instead, we are 
interested in using (3) as an exemplary solution from which we shall draw 
several very general conclusions. 

We should note first that, for a source-free circuit, Q must be zero, 
and the solution is the natural response 

in = Ae- pt (4) 

We shall find that the constant P is never negative; its value depends only 
on the passive circuit elements 3 and their interconnection in the circuit. 
The natural response therefore approaches zero as time increases without 
limit. It must do so, of course, in the simple RL series circuit because the 
initial energy is gradually dissipated in the resistor. There are also idealized, 
nonphysical circuits in which P is zero; in these circuits the natural response 
does not die out, but approaches a constant value, as exemplified by trapped 
currents or voltages. We therefore find that one of the two terms making 
up the complete response has the form of the natural response; it has an 
amplitude which will depend on the initial value of the complete response 
and thus on the initial value of the forcing function also. 

We next observe that the first term of (3) depends on the functional 
form of Q(t), the forcing function. Whenever we have a circuit in which 
the natural response dies out as t becomes infinite, then this first term must 
describe the form of the response completely after the natural response 
has disappeared. This term we shall call the forced response; it is also called 
the steady-state response, the particular solution, or the particular integral. 

For the present, we have elected to consider only those problems 
involving the sudden application of dc sources, and Q(t) is therefore a 
constant for all values of time after the switch has been closed. If we wish, 
we can now evaluate the integral in (3), obtaining the forced response 


3 If the circuit contains a dependent source or a negative resistance, it is possible for P to 
be negative. 

1 82 ^' 1e T ™ n *'» n ' Circuit 

or the complete response 

i(t) =£ + Ae~" 

For the RL series circuit, Q/P is the constant current V/R and 1/P is the 
time constant t. We should see that the forced response might have been 
obtained without evaluating the integral, because it must be the complete 
response at infinite time; it is merely the source voltage divided by the 
series resistance. The forced response is thus obtained by inspection. 

In the following section we shall attempt to find the complete response 
for several RL circuits by obtaining the natural and forced responses and 
then adding them. 

Drill Problem 

6-4 Let the voltage source 6e~ 2t u(t) V be connected in series with a 2-H inductor 
and a 10-fi resistor. Using (3), determine i at t = : (a) + ; (b) 0.2 s; (c) 0.5 s. 

Ans. 0; 0.286; 0.302 A 


Let us use the simple RL series circuit to illustrate how to determine the 
complete response by the addition of the natural and forced responses. 
This circuit, shown in Fig. 6-10, has been analyzed earlier, but by a longer 
method. The desired response is the current i(t), and we first express this 
current as the sum of the natural and the forced current, 


The functional form of the natural response must be the same as that 
obtained without any sources. We therefore replace the step-voltage source 

Fig. 6-10 A series RL circuit which is used to illustrate the method by 
which the complete response is obtained as the sum of the natural and forced 

183 The Application of Hi* Unit-»tep Forcing FuncNon 

by a short circuit and recognize the old RL series loop. Thus, 

i n = Ae- Rt/L 

where the amplitude A is yet to be determined. 

We next consider the forced response, that part of the response which 
depends upon the nature of the forcing function itself. In this particular 
problem the forced response must be constant because the source is a 
constant V for all positive values of time. After the natural response has 
died out, therefore, there can be no voltage across the inductor; hence, 
a voltage V appears across R, and the forced response is simply 


Note that the forced response is determined completely; there is no un- 
known amplitude. We next combine the two responses 

: Ae- 

and apply the initial condition to evaluate A. The current is zero prior 
to t — 0, and it cannot change value instantaneously since it is the current 
flowing through an inductor. Thus, the current is zero immediately after 

t = 0, and 

0-A + J 



L ) 


This response is plotted in Fig. 6-11, and we can see the manner in 
which the current builds up from its initial value of zero to its final value 

Fig. 6-1 1 The current expressed by (5) is shown graphically. A line extend- 
ing the initial slope meets the constant forced response at t = T. 


0.632 V/B V-. 




so vi 6 a ; 

Fig. 6-12 A circuit used as an example. 

of V/R. The transition is effectively accomplished in a time 3t. If our 
circuit represents the field coil of a large dc motor, we might assign 
L = 10 H and JR = 20 ft, obtaining t = 0.5 s. The field current is thus 
established in about 1.5 s. In one time constant, the current has attained 
63.2 per cent of its final value. 

Now let us apply this method to a more complicated circuit. In Fig. 
6-12, there is shown a circuit containing a dc voltage source as well as 
a step-voltage source. Let us determine i(t) for all values of time. We might 
choose to replace everything to the left of the inductor by the Thevenin 
equivalent, but instead let us merely recognize the form of that equivalent 
as a resistor in series with some voltage source. The circuit contains only 
one energy-storage element, the inductor, and the natural response is 
therefore a negative exponential as before, 

» = *r + K 

i„ = Ae- t/2 t > 

*„ 1-5 

The forced response must be that produced by a constant voltage of 
100 V. The forced response is constant, and no voltage is present across 
the inductor; it behaves as a short circuit and, therefore, 


i = 50 + Ae" 05 ' t > 

In order to evaluate A, we must establish the initial value of the inductor 
current. Prior to t = 0, this current is 25 A, and it cannot change instan- 
taneously. Thus, 

25 = 50 + A or A = -25 







» t (») 

Hg. 6-13 The response «(t) of the circuit shown in Fig. 6-12 is sketched for 
values of time less and greater than zero. 


» = 50 - 25e-°- 5 ' t > 

We complete the solution by also stating 

i = 25 t < 
or by writing a single expression valid for all t, 

i = 25 + 25(1 - e-°- 5 ')u(t) A 

The complete response is sketched in Fig. 6-13. Note how the natural 
response serves to connect the response for ( < with the constant forced 

As a final example of this method by which the complete response of 
any circuit subjected to a transient may be written down almost by inspec- 
tion, let us apply a rectangular voltage pulse of amplitude V and duration 
t to the simple RL series circuit. We represent the forcing function as 
the sum of two step-voltage sources Vu(t) and — Vu(t — t ), as indicated 
in Fig. 6- 14a and b, and plan to obtain the response by using the super- 

Fig. 6-14 (a) A rectangular voltage pulse which is to be used as the forcing 
function in a simple series RL circuit, {b) The series RL circuit, showing the 
representation of the forcing function by the series combination of two inde- 
pendent voltage-step sources. The current s(£) is desired. 






1 + R 


Vu «)(\) 



-Vu(« - *o»(l) 




1 86 * ne Transient Circuit 

position principle. Suppose we designate that part of i(t) which is due to 
the upper source Vuit) acting alone by the symbol i t (t) and then let i 2 (t) 
represent that part due to — Vu(t — t ) acting alone. Then, 

i(t) = i^t) + i 2 (t) 

Our object is now to write each of the partial responses i x and i 2 as the 
sum of a natural and a forced response. The response t 1 (t) is familiar; this 
problem was solved two or three pages back, 



L ) t>0 

Note that the range of t, t > 0, in which this solution is valid, is indicated. 
We now turn our attention to the lower source and its response i 2 (t). 
Only the polarity of the source and the time of its application are different. 
There is thus no need to determine the form of the natural response and 
the forced response; the solution for t 1 (() enables us to write 

'#)= -|(l-^ ( '-' ol/t ) t>t 

where the applicable range of t, t > t , must again be indicated. 

We now add the two solutions, but do so carefully, since each is valid 
over a different interval of time. Thus, 

Kt) = £(1 - e-«' /L ) 0<t<t 

i(t) = |(1 - e- R%,L ) - ^(1 - e -*'-'o>/i) t > t 

m = 



1) t > t 

Fig. 6-15 Two possible response curves are shown for the circuit of Fie 
6-1 4b. In {a), t is selected as t /"2, and in {b) as 2t . 



5> t 


1 g7 The Application of the Unit-itep Forcing Function 

The solution is completed by stating that i(t) is zero for negative t and 
sketching the response as a function of time. The type of curve obtained 
depends upon the relative values of t and the time constant t. Two possible 
curves are shown in Fig. 6-15. The left curve is drawn for the case where 
the time constant is only one-half as large as the length of the applied pulse; 
the rising portion of the exponential has therefore almost reached V/R 
before the decaying exponential begins. The opposite situation is shown 
to the right; there, the time constant is twice t and the response never 
has a chance to reach the larger amplitudes. 

Drill Problems 

6-5 Find the forced portion of the response i(t) for the circuits of Fig. 6-16a, 

b, and c. 

Ans. 2; 4; 6 A 

• (DM sn 


Fig. 6-16 See Drill Probs. 6-5, 6-6, and 6-7. 

6-6 Find the value of t(0 + ) for the circuits of Fig. 6-16a, b, and c. 

Ans. 2; 2.5; 6 A 

6-7 Find i(t) for f > for the circuits of Fig. 6-16a, b, and c. 

Ans. 2 + 0.5e-" 2 ; 4 + 2e~ tn ; 6 - 4e'" 2 A 

188 Th * Transient Clrcuil 

The complete response of any RC circuit may also be obtained as the sum 
of the natural and the forced response. We shall consider several responses 
in the circuit shown in Fig. 6-17. The switch is assumed to have been in 
position "a" for a long time, or, in other words, the natural response which 
resulted from the original excitation of the circuit has decayed to a negligi- 
ble amplitude, leaving only a forced response caused by the 120-V source. 
We are asked for v^t), and we thus begin by finding this forced response 
when the switch is in position "a." The voltages throughout the circuit 
are all constant, and there is thus no current through the capacitor. Simple 
voltage division determines the forced response prior to t = 0, 


" w ~ 50 + 10 

120 = 100 t < 

and we thus have the initial condition 

o c (0) = 100 

Since the capacitor voltage cannot change instantaneously, this voltage is 
equally valid at t = 0~ and t = + . 

The switch is now thrown to "b," and the complete response is 

V C = *>Cf + v c 

The form of the natural response is obtained by replacing the 50-V source 
by a short circuit and evaluating the equivalent resistance, 




ISO + /200 + /60 


Fig. 6-17 An RC circuit in which the complete responses v c and i are ob- 
tained by adding a forced response and a natural response. 

1 39 Th * Application of Hio Unit-stop Forcing Function 

In order to evaluate the forced response with the switch at "b," we wait 
until all the voltages and currents have stopped changing, thus treating 
the capacitor as an open circuit, and use voltage division once more, 

(50)(200)/(50 + 200) 
D °' ~ 60 + (50)(200)/(50 + 200) 

50 = 20 


20 + Ae-' n - 2 

and from the initial condition already obtained, 

100 = 20 + A 
or c c = 20 + 80e- ,/12 t > 

This response is sketched in Fig. 6-18a; again the natural response is seen 
to form a transition from the initial to the final response. 

Finally, let us calculate some response that need not remain constant 
during the instant of switching, such as i(t) in Fig. 6-17. With the contact 
at a, it is evident that i = 50 / 26O — 0.192 A. When the switch is in position 
b, the forced response for this current now becomes 



60 + (50)(200)/(50 + 200) 50 + 200 

= 0.1 

The form of the natural response is the same as that we already determined 
for the capacitor voltage, 

i„ = Ae-' n - 2 

Combining the forced and natural responses, we obtain 

i = 0.1 + Ae~' n - 2 

Fig. 6-18 The responses [a) v c and [b) i are plotted as functions of time 
for the circuit of Fig. 6-17. 


3 t (s) 






1 T 2 3 l'<«) 


1 90 The Transient Circuit 

To evaluate A, we need to know t(0+). This is found by fixing our attention 
on the energy-storage element, here the capacitor, for the fact that v c must 
remain 100 V during the switching interval is the governing condition 
establishing the other currents and voltages at t = + . Since v c (0 + ) — 
100 V, and since the capacitor is in parallel with the 200-0 resistor, we 
find t(0 + ) = 0.5 A, A = 0.4, and thus, 

»(*) = 0.192 r<0 
i{t) = 0.1 + 0.4e- (/1 - 2 t > 
or i(«) = 0.192 + (-0.092 + 0.4e- (/1 - 2 )u(f) A 

where the latter expression is correct for all t. 

The complete response for all t may also be written concisely by using 
u( — t), which is unity for t < and for t > 0. Thus, 

i(t) - 0.192u(-t) + (0.1 + 0Ae-' n - 2 )u(t) A 

This response is sketched in Fig. 6-18i>. Note that only four numbers are 
needed to write the functional form of the response for this single en- 
ergy-storage-element circuit or to prepare the sketch: the constant value 
prior to switching (0.192 A), the instantaneous value just after switching 
(0.5 A), the constant forced response (0.1 A), and the time constant (1.2 s). 
The appropriate negative exponential function is then easily written or 


□ 1 Sketch each of the following waveforms as functions of time and calculate 
its value at t = 2 s: (a) u(t + 3) - u(t - 3); (b) u(3 + t) - «(3 - t); (c) tult) + 
u(t - 1.5) - (t - S)u(t - 3); (d) e-'u(t) - e- x u(f - 1); (e) u(t - t 2 ). 

□ 2 A 1.5-V battery, a 30-S2 resistor, and an open switch are in series. The switch 
closes at t = 0, opens at t = 1 s, closes at t = 2 s, and continues in the same 
pattern thereafter. Express the current as an infinite summation of step functions. 

□ 3 Find the current entering the upper conductor of each of the general networks 
shown in Fig. 6-3 if V = 20 V, t = 2 s, and the general network consists of a 
5-£2 resistor in series with a 5-V (ideal) battery being charged. 

□ 4 The current, i(t) = 20u(f) — 20«(* - 10" 3 ) mA, is applied to a 10-/iF capaci- 
tor. Find the capacitor voltage as a function of time, and evaluate your result 
at t = 0.5 and 2 ms. 

|9] The Application of the Unit-step Forcing Function 

□ 5 A 2-H inductor, a 50-12 resistor, and the series combination of a 100-12 resistor 
and an independent voltage source 45u(t) V are all in parallel, (a) Replace 
everything except the inductor by its Thevenin equivalent and find the inductor 
current as a function of time, (b) Repeat for the Norton equivalent. 

□ 6 A 10-12 resistor, a 5-H inductor, and an independent voltage source are in 
series. Find and sketch the current if the source voltage is: (a) 50 — 50u(t) V; 
(b) 50 + 50u(t) V; (c) 50 + 50u(f) - 100«(t - 1) V. 

□ 7 Through the use of an exponential integrating factor, solve the differential 
equation for the current if a series circuit consists of a 10-12 resistor, a 1-H inductor, 
and an independent voltage source: (a) 2 cos lOt u(t) V; (b) It u(t) V. 

□ 8 For the circuit shown in Fig. 6-19, find: (a) i L ; (b) v L . 

24u(l) V 

Fig. 6-19 See Probs. 8 and 9. 

□ 9 Change the label on the voltage source in Fig. 6-19 from 24u(t) to 12 — 
24u(t) V and rework Prob. 8. 

D 1 In the circuit shown in Fig. 6-20, the switch has been in the position shown 
for a long time. At t = it is moved to the left. Find and sketch i L (t). 

2A(t) 40 n 

4fi (1")2A 

Fig. 6-20 See Prob. 10. 
□ 1 1 For the circuit of Fig. 6-21, let i s = 2u(t) A and find: (a) i L ; (b) i v 

Fig. 6-21 See Probs. 11 to 13. 


1 92 T*" Transient Circuit 

D 12 For the circuit of Fig. 6-21, let t, = -2u(t) A and find: (a) i L ; (b) i v 
□ 13 For the circuit of Fig. 6-21, let i, = -2 A and find: (a) i L ; lb) i v 
D 14 Find i x (*), i 2 (t), and v 3 (t) for the circuit illustrated by Fig. 6-22. 

Fig. 6-22 See Prob. 14. 

D 1 5 Find the voltage across each of the three passive circuit elements in Fig. 
6-23 at t = 0+ if u, = : (a) 0; \b) 12 V; (c) 12u(f) V. 


Fig. 6-23 See Prob. 1 5. 

□ 16 For the circuit shown in Fig. 6-24, find and sketch as functions of time: (a) 

iM (b) i R (t)- 

Fig. 6-24 See Prob. 16. 
D 17 For the circuit shown in Fig. 6-25, find i L (t). 

D 18 A 60u(f)-V source, a 6-fl resistor, and a 6-H inductor are in series. At t = 1 s, 
a 3-H inductor is suddenly connected in parallel with the 6-H inductor. Find, as 
functions of time: (a) the source current; (b) the 6-H inductor current. 

D 19 If a 20-ki2 resistor, a 10-f»F capacitor, and the parallel combination of a 10-kfl 

Fig. 6-25 See Prob. 17. 

resistor and an independent current source of 6u(t) mA are all in series, find: (a) 
the capacitor voltage; (b) the current through the 10-kfl resistor. 

DMA 20-/iF capacitor, a 25-kfl resistor, and an independent current source are 
in parallel. Find the capacitor voltage v^t) if the source current is: (a) 4[1 — 
«(r)] mA; (b) 4[1 + u(t)] mA. 

D 21 For the circuit shown in Fig. 6-26, find v^t) and i^t) if i, = : (a) 25u(r) mA; 
(b) 10 + 15u(r) mA. 

Hg. 6-26 See Prob. 21. 

□ 22 With reference to the circuit shown in Fig. 6-27, let t>, = 30u(t) V and 
determine: (a) o^t); (b) v t (t). 


10 mF" go ln 
f + ^ lOkfl^"! (T)3«(()mA 

Rg. 6-27 See Probs. 22 and 23. 

D 23 Let c, = -30u(f) V in the circuit of Fig. 6-27. Find: (a) v^t); (b) v^t). 

a 24 For the circuit shown in Fig. 6-28, let c, = and find: (a) v^t); (b) v 2 (t); 
(c) < 3 W- 

D 25 For the circuit shown in Fig. 6-28, let i), = 4V and find: (a) v^t); (b) c 2 (r); 
(c) i 3 (t). 


20 kn ' = o 
-W* — t— "V- 

». f± J '3 >20 kfi 

0.03 ^F £40kfi + 1 

- 0.01 juF 


Fig. 6-28 See Probs. 24 and 25. 

D 26 Find iffi), i 2 (0+), and i 3 (0+) in the circuit shown in Fig. 6-29 if i s = 

0; (b) 3 A; (c) 3u(t) A. 


48 11(0/ 

'l. »2 

6 juF I 2 Q L |i 3 

••„(T) say 


Fig. 6-29 See Prob. 26. 

D 27 For the circuit shown in Fig. 6-30, find u c (t) if the dependent source is labeled 
v s = : (a) 500i i; (b) 0.5c c . 



50„«)^\ '^ lkJ , Irf^tcli) 

Fig. 6-30 See Prob. 27. 


Chapter Seven 
The RLC Circuit 


It would be very pleasant to learn that the detailed study we have just 
completed for the RL and RC circuits will make the analysis of the RlJC 
circuit a simple task; unfortunately the analysis remains difficult. The 
presence of inductance and capacitance in the sanie circuit produces at 
least a second-order system, that is, one that is characterized by a linear 
differential equation including a second-order derivative, or by two simul- 
taneous linear 6rst-order differential equations. Although we have con- 
sidered one second-order system in the final section of Chap. 5, most 
of our attention has been directed toward the first-order system which is 

1 96 Th * Tran > i * n * Circuit 

described by a first-order linear differential equation. From the single 
case we have considered, we should suspect that this increase in order 
will make it necessary to evaluate two arbitrary constants. Furthermore, 
it will be necessary to determine initial conditions for derivatives. And 
finally, we shall see that the presence of inductance and capacitance in 
the same circuit leads to a response which takes on different functional 
forms for circuits which have the same configuration but different element 
values. With this cheerful news, let us quickly review the methods and 
results we found useful for first-order systems, in order that we may ex- 
tend this information as intelligently as possible to the second-order 

We first considered the source-free first-order system. The response was 
termed the natural response, and it was determined completely by the types 
of passive elements in the network, by the manner in which they were 
interconnected, and by the initial conditions which were established by 
the stored energy. The natural response was invariably an exponentially 
decreasing function of time, and this response approached a constant value 
as time became infinite. The constant was usually zero, except in those 
circuits where paralleled inductors or series-connected capacitors allowed 
trapped currents or voltages to appear. 

The addition of sources to the first-order system resulted in a two-part 
response, the familiar natural response and an additional term we called 
the forced response. This latter term was intimately related to the forcing 
function; its functional form was that of the forcing function itself, plus 
the integral and first derivative of the forcing function. 1 Since we treated 
only a constant forcing function, we have not needed to devote much 
attention to the proper form of the forced response; this problem will not 
arise until sinusoidal forcing functions are encountered in the following 
chapter. To the known forced response, we added the correct expression 
for the natural response, complete except for a multiplicative constant. 
This constant was evaluated to make the total response fit the prescribed 
initial conditions. 

We now turn to circuits which are characterized by linear second-order 
differential equations. Our first task is the determination of the natural 
response. This is most conveniently done by considering initially the 
source-free circuit. We may then include dc sources, switches, or step 
sources in the circuit, representing the total response once again as the 
sum of the natural response and the (usually constant) forced response. 
The second-order system that we are about to analyze is fundamentally 
the same as any lumped-constant mechanical second-order system. Our 

higher-order derivatives will appear in higher-order systems, and, strictly speaking, we 
should say that all derivatives are present, although possibly with zero amplitude. Forcing 
functions which do not possess a finite number of different derivatives are exceptions which 
we shall not consider; the singularity functions are exceptions to the exceptions. 

1 97 Th* R1C Circuit 

results, for example, will be of direct use to a mechanical engineer who 
is interested in the displacement of a spring-supported mass subjected to 
viscous damping, or one who is interested in the behavior of a simple 
pendulum or a torsional pendulum. Our results are still applicable, although 
less directly, to any distributed-parameter second-order system, such as a 
short-circuited transmission line, a diving board, a flute, or the ecology of 
the lemming. 


Our first goal is the determination of the natural response of a simple circuit 
formed by connecting R, L, and C in parallel; this modest goal will be 
reached after completing this and the next three sections. This particular 
combination of ideal elements is a suitable model for portions of many 
communications networks. It represents, for example, an important part 
of some of the electronic amplifiers found in every radio receiver, and it 
enables the amplifiers to produce a large voltage amplification over a 
narrow band of signal frequencies and nearly zero amplification outside 
this band. Frequency selectivity of this kind enables us to listen to the 
transmission of one station while rejecting the transmission of any other 
station. Other applications include the use of parallel RLC circuits in 
multiplexing filters, harmonic suppression filters, and so forth. But even 
a simple discussion of these principles requires an understanding of such 
terms as resonance, frequency response, and impedance which we have 
not yet discussed. Let it suffice to say, therefore, that an understanding 
of the natural behavior of the parallel RLC circuit is fundamentally impor- 
tant to future studies of communications networks and filter design. 

When a physical inductor is connected in parallel with a capacitor, and 
the inductor has associated with it a nonzero ohmic resistance, the resulting 
network can be shown to have an equivalent circuit model like that shown 
in Fig. 7-1. Energy losses in the physical inductor are taken into account 
by the presence of the ideal resistor whose resistance R is dependent upon 
(but not equal to) the ohmic resistance of the inductor. 

In the following analysis we shall assume that energy may be stored 

Fig. 7-1 The source-free parallel RLX2 circuit. 


1 98 The Transient Circuit 

initially in both the inductor and the capacitor, and thus nonzero values 
of both inductor current and capacitor voltage are initially present. With 
reference to the circuit of Fig. 7-1, we may then write the single nodal 

c If'. , ■. „dv 


Note that the minus sign is a consequence of the assumed direction for 
i. We must solve (1) subject to the initial conditions 

m = /„ (2) 

«(0 + ) = V (3) 

When both sides of (1) are differentiated once with respect to time, the 
result is the linear second-order homogeneous differential equation 

whose solution v(t) is the desired natural response. 

There are a number of interesting ways to solve (4). These methods 
we shall leave to a course in differential equations, selecting only the 
quickest and simplest method to use now. We shall assume a solution, 
relying upon our intuition and modest experience to select one of the several 
possible forms which are suitable. Our experience with the first-order 
equation should suggest that we at least try the exponential form once 
more. Moreover, the form of (4) indicates that this may work, because 
we must add three terms, the second derivative, first derivative, and the 
function itself, each multiplied by a constant factor, and achieve a sum 
of zero. A function whose derivatives have the same form as the function 
itself is obviously a sensible choice. With every hope for success, then, 
we assume 

v = Ae s < (5) 

where we shall be as general as possible by allowing A and s to be complex 
numbers if necessary. 2 Substituting (5) into (4), we obtain 

CAjsV + l-Ase*' + —Ae st = 
R L 

At** (cs 2 + ±s + j) = 

2 There is no cause for panic. Complex numbers will appear in this chapter only in an 
introductory way in the derivations. Their use as a tool will be necessary in Chap. 9. 

1 99 The R1C Circuit 

In order for this equation to be satisfied for all time, one of the three 
factors must be zero. If either of the first two factors is put equal to zero, 
then v(t) = 0. This is a trival solution of the differential equation which 
cannot satisfy our given initial conditions. We therefore equate the re- 
maining factor to zero, 

C* + ± + f = (6) 

This equation is usually called the auxiliary equation or the characteristic 
equation by mathematicians. If it can be satisfied, then our assumed solution 
is correct. Since (6) is a quadratic equation, there are two solutions, 
identified as s 1 and s 2 , 


Sl 2RC + V\2flcj LC 

and * 2= _ 2flC~VV2fic) ~LC (8) 

If either of these two values is used for s in the assumed solution, then 
that solution satisfies the given differential equation; it thus becomes a valid 
solution of the differential equation. 

Let us assume that we replace s by s x in (5), obtaining 

Vl = Aje 81 ' 

and, similarly, 

v 2 = A 2 e**> 

The former satisfies the differential equation 

„ d 2 v, 14 1 

c -5F + H-* + r'i = 

and the latter satisfies 

„d 2 v 9 1 dvo 1 

Adding these two differential equations and combining similar terms, 

° dt 2 R dt L K 1 T 2 ' 

linearity triumphs, and it is seen that the sum of the two solutions is also 

200 * ne Transient Circuit 

a solution. We thus have the form of the natural response 

v = A^ 1 ' + A 2 e" 2 ' (9) 

where s 1 and s 2 are given by (7) and (8), and A 1 and A 2 are two arbitrary 
constants which are to be selected to satisfy the two specified initial 

The form of the natural response as given above can hardly be expected 
to bring forth any expressions of interested amazement, for, in its present 
form, it offers little insight into the nature of the curve we might obtain 
if v(t) were plotted as a function of time. The relative amplitudes of A x 
and A 2 , for example, will certainly be important in determining the nature 
of the response curve. Furthermore, the constants s r and s 2 can be real 
numbers or conjugate complex numbers, depending upon the values of R, 
L, and C in the given network. These two cases will produce fundamentally 
different response forms. Therefore it will be helpful to make some simpli- 
fying substitutions in (9) for the sake of conceptual clarity. 

Since the exponents s^ and s 2 t must be dimensionless, Sj and s 2 must 
have the unit of some dimensionless quantity "per s econ d." From (7) and 
(8) it is apparent that the units of 1/2RC and 1/yJLC must also be s -1 . 
Units of this type are called frequencies. Although we shall expand 
this concept in much more detail in Chap. 13, we shall introduce several 
of the terms now. Let us represent 1/VEC by w (omega), 



and reserve the term resonant frequency 3 for it. On the other hand, we 
shall call 1/2RC the neper frequency or the exponential damping coefficient 
and represent it by the symbol a (alpha), 

a = 25c <»> 

This latter descriptive expression is used because a is a measure of how 
rapidly the natural response decays or damps out to its steady final value 
(usually zero). Finally, s, s x , and s 2 , which are quantities that will form 
the basis for some of our later work, will be called complex frequencies. 
Let us collect these results. The natural response of the parallel RLC 
circuit is 

v(t) = Aje 8 ' 1 + A 2 e* 2 ' (9) 

3 More accurately, the resonant radian frequency. 

201 The MC Circuit 


«!=-«+ V<* 2 - u 2 

s 2 = -a - V« 2 - <">o 2 

a = mc 





and A x and A 2 must be found by applying the given initial conditions. 
It is now apparent that the nature of the response depends upon the 
relative magnitudes of a and u . The radical appearing in the expressions 
for Sj and s 2 will be real when a is greater than <o , imaginary when a 
is less than <o , and zero when a and <o are equal. Each of these cases 
will be considered separately in the following three sections. 

Drill Problem 

7-1 Determine values for a, w , and s 1 for a parallel RLC circuit in which 
C = 0.1 M F, fi = 1 kfi, and L = : (a) 0.625 H; (b) 0.4 H; (c) 0.256 H. 

Arts. 5, 4, -2; 5, 5, -5; 5, 6.25, -5 + J3.75 (ms)" 1 


It is apparent that a will be greater than <o and a 2 will be greater than 
<o 2 if LC> 4R 2 C 2 . In this case the radical we are concerned with will 
be real, and both s t and s 2 will be real. Moreover, the following inequalities, 


(-a - V« 2 - «>o 2 ) < (-« + V« 2 - <V) < 

may be applied to (12) and (13) to show that both s 1 and s 2 are negative 
real numbers. Thus, the response v(t) can be expressed as the (algebraic) 
sum of two decreasing exponential terms, both of which approach zero 
as time increases without limit. In fact, since the absolute value of s 2 is 
larger than that of s lt the term containing s 2 has the more rapid rate of 
decrease and, for large values of time, we may write the limiting expression 

v(t) -> Aje*' 1 -> as t -> oo 

In order to discuss the method by which the arbitrary constants A x and 


Fig. 7-2 A parallel RLC circuit used as a numerical example. The cir- 
cuit is overdamped. 

A 2 are selected to conform with the initial conditions, and in order to 
provide a typical example of a response curve, let us turn to a numerical 
example. We shall select a parallel RLC circuit for which R = 6 Q, 
L = 7 H, and, for ease of computation, the unpractically large value 
C = /42 F ' th e initial energy storage is specified by choosing an initial 
voltage across the circuit «(0) = and an initial inductor current t(0) = 
10 A, as shown in Fig. 7-2. 

We may easily determine the values of the several parameters 

a = 3.5 
Sl = -1 

= Ve 

(all s- 1 ) 

and immediately write the general form of the natural response 

v(t) = A x e"' + A 2 e- 6 ' 


Only the evaluation of the two constants A 1 and A 2 remains. If we knew 
the response v(t) at two different values of time, these two pairs of values 
could be substituted in (14) and A 1 and A 2 easily found. However, we know 
only the initial value of v(t), 

€(0) = 

and, therefore, 

= A, + A, 


A second equation relating A x and A 2 must be obtained by taking the 
derivative of v(t) with respect to time in (14), determining the initial value 
of this derivative through the use of the remaining initial condition t(0) = 
10, and equating the results. Taking the derivative of both sides of (14), 


= -Aje-' - 6A 2 e~ 


203 The Rlc c ' rcuit 

evaluating the derivative at t = 0. 

dv I 
dt I ,_„ 

= -A r - 6A. 

we next pause to consider how the initial value of the derivative can be 
found numerically. This next step is always suggested by the derivative 
itself; dv/dt suggests capacitor current, for 


c dt 

dv 1 
dt \ 

iJP) «(0) + 1,(0) _ i(0) 
(=o C C C 

= 420 V/s 

since zero voltage across the resistor requires zero current through it. We 
thus have our second equation 

420 = -A t - 6A 2 (16) 

and simultaneous solution of (15) and (16) provides the two amplitudes 
A 2 = 84 and A 2 = — 84. Thus, the final numerical solution for the natural 
response is 

u(t) = 84(e-' - e- 6 ') (17) 

The evaluation of A x and A 2 for other conditions of initial energy storage, 
including initial energy storage in the capacitor, is considered in the first 
drill problem following this section. 

Let us see what information we can glean from (17) without calculating 
unduly. We note that v(t) is zero at t = 0, a comforting check on our 
original assumption. We may also interpret the first exponential term as 
having a time constant of 1 s and the other exponential, a time constant 
of Y 6 s. Each starts with unity amplitude, but the second decays more 
rapidly; v(t) is thus always positive. As time becomes infinite, each term 
approaches zero, and the response itself dies out as it should. We thus have 
a response curve which is zero at t = 0, zero at t = oo, and is always 
positive; since it is not everywhere zero, it must possess at least one 
maximum, and this is not a difficult point to determine exactly. We differ- 
entiate the response 

4r- = 84(-e-' + 6e~ 6 ') 

204 The Transient Circuit 

set the derivative equal to zero to determine the time t m at which the 
voltage becomes maximum, 

manipulate once, 
and obtain 

= -e-'" + 6e- 6< » 

t m = 0.358 s 
v(t m ) = 48.9 V 

A reasonable sketch of the response may be made by plotting the two 
exponential terms 84e~' and 84e -6 ' and then taking their difference. The 
usefulness of this technique is indicated by the curves of Fig. 7-3; the two 
exponentials are shown lightly, and their difference, the total response v(t), 
is drawn with a heavier line. The curves also verify our previous prediction 
that the functional behavior of v(t) for very large t is 84e~ ( , the exponential 
term containing the smaller magnitude of s x and s 2 . 

Another question that frequently arises in the consideration of network 
response is concerned with the length of time it takes for the transient 
part of the response to disappear (or damp out). In practice, it is often 
desirable to have this transient response approach zero as rapidly as possi- 
ble, that is, to minimize the settling time t s . Theoretically, of course, t„ 
is infinite, because v(t) never settles to zero in a finite time. However, 
a negligible response is present after v(t) has settled to values that are less 
than 1 per cent of its maximum value v m . The time which is required for 
this to occur we define as the settling time. Since v m is 48.9 V for our 
example, the settling time is the time required for the response to drop 

Fig. 7-3 The response v{t) ■■ 
shown in Fig. 7-2. 

: 84|e-' - e- & ) of the network which 

>l (»> 

205 Th * R1C Circui * 

to 0.489 V. Substituting this value for v(t) into (17) and neglecting the 
second exponential term, known to be negligible here, the settling time is 
found to be 5.15 s. 

In comparison with the responses which we shall obtain in the following 
two sections, this is a comparatively large settling time; the damping takes 
overly long, and the response is called overdamped. We shall refer to the 
case for which a is greater than <o as the overdamped case. Now let us 
see what happens as a is decreased. 

Drill Problems 

7-2 If the initial voltage across a parallel RLC circuit is not zero, then the 
resultant value of the initial resistor current must be considered in evaluating 
the initial value of dv/dt. For the numerical example considered in the above 
section, determine A t and A 2 for the following initial conditions: (a) c(0) = 10 V, 
i(0) = 10 A; (b) u(0) = 10 V, i(0) = - 10 A; (c) o(0) = 24 V, t(0) = 2 A. 

Am. -86, 96; 12, 12; 82, -72 V 

7-3 Given a parallel RLC circuit in which R = 400 fi, C = 0.01 jiF, and L = 
10 mH, determine the voltage across the circuit at the times indicated below 
if the initial values are u(0) = 20 V, i(0) = 20 mA: (a) t = 2 /is; (b) t = 5 us; (c) 
t = 20 /is. 

Ans. 2.70; 10.1; 15.0 V 


The overdamped case is characterized by 

« >«o 
or LC > 4R 2 C 2 

and leads to negative real values for * x and s 2 and to a response expressed 
as the algebraic sum of two negative exponentials. Typical forms of the 
response v(t) are obtained through the numerical example in the last section 
and in the drill problems following it. 

Now let us adjust the element values until a and w are equal. This 
is a very special case which is termed critical damping. Thus, critical 
damping is achieved when 

a = w„ 

or LC = 4fi 2 C 2 

or L = 4fl 2 C J 

critical damping 

206 Tne Transient Circuit 

It is obvious that we may produce critical damping by changing the value 
of any one of the three elements in the numerical example discussed above. 
We shall select R, increasing its value until critical damping is obtained, 
and thus leave to unchanged. The necessary value of R is 7\/6/2 Q; L 
is still 7 H, and C remains % 2 F. We thus find 

a = o> = \/6 
Sj = s 2 = — \/6 

and we blithely construct the response as the sum of the two exponentials, 

v(t) = A ie -^' + A 2 e~^ 
which may be written as 

v(t) = A 3 e~^> 

At this point, some of us should feel we have lost our way. We have 
a response which contains only one arbitrary constant, but there are two 
initial conditions v(0) = and i(0) = 10 which must be satisfied by this 
single constant. This is in general impossible. In our case, for example, 
the first initial condition requires A 3 to be zero, and it is then impossible 
to satisfy the second initial condition. 

Our mathematics and our electricity have been unimpeachable; there- 
fore, if a mistake has not led to our difficulties, we must have begun with 
an incorrect assumption, and only one assumption has been made. We 
originally hypothesized that the differential equation could be solved by 
assuming an exponential solution, and this turns out to be incorrect for 
this single special case of critical damping. We must therefore return to 
the differential equation and attempt to solve it by some other means than 
an assumed solution. Although this detailed solution is carried out below, 
we should realize that it is the final functional form of the response which 
is important to us, and not the specific method by which it is obtained. 
After all, if we were clever enough, we could assume a response of the 
correct form and then check it by direct substitution in the differential 

The original differential equation, (4), 

r d 2 v , 1 dv , 1 _ n 
may be written in terms of a and w , 
dt 2 + la dt 

207 The RlC Circuit 

which becomes, for critical damping, 

4* + 2a% + cflv = 
at* at 

or ^f + a d!L + a <^ + a 2 v = 

at* at at 

and finally, 

If we now let 


£(£H + -(£ + ~)=° 

. = £ + « 

which is a form we have encountered before. Its solution is 

and, therefore, 


4°- + av = A ie -" 

This equation has the form of Eq. (6-2), and therefore we should be able 
to solve it by the use of an integrating factor. The integrating factor is 
e +at , and we multiply both sides of the equation by it, 

recognize the derivative of the product and simplify, 

Finally, we integrate each side directly, 

ue"' = A x t + A 2 
and obtain the desired response form 

v = e-'-'iAjt + A 2 ) (18) 

208 * n * Transient Circuit 

It should be noted that the solution may be expressed as the sum of two 
terms, where one term is the familiar negative exponential but the second 
is t times a negative exponential. We should also note that the solution 
contains the two expected arbitrary constants. 

Let us now complete our numerical example. After we substitute the 
known value of a into (18), 

v = Ajte - ^' + A 2 , 


we establish the values of A t and A 2 by first imposing the initial condition 
on v(t) itself, t>(0) = 0. Thus, A 2 = 0. This simple result occurs because 
the initial value of the response was selected as zero; the more general 
case, which leads to an equation determining A 2 , may be expected to arise 
in the drill problems. The second initial condition must be applied to the 
derivative dv/dt just as in the overdamped case. We therefore differentiate, 
remembering that A 2 = 0, 

^ = A 1 t(- V6)e-v® + Ai e-Vf» 

evaluate at t = 0, 

dv \ _ A 

express the derivative in terms of the initial capacitor current, 

*i| _. »c(0) ^ <«(0) , <(0) 
dt ! t=0 C C C 

and thus 

A 1 = 420 
The response is, therefore, 

v(i) = 420te- 245t (19) 

Before plotting this response in detail, let us again try to anticipate 
its form by qualitative reasoning. The specified initial value is zero, and 
(19) concurs. It is not immediately apparent that the response also ap- 
proaches zero as t becomes infinitely large because te~ 2A5t is an indeter- 
minate form. However, this minor obstacle is easily overcome by use of 
L'H6pital's rule. Thus, 

209 Tha Rlc Circuit 

lim v(t) 


420 lim 

= 420 lim 

2.45e 2 - 45 ' 


and once again we have a response which begins and ends at zero and 
has positive values at all other times. A maximum value v m again occurs 
at time t m ; for our example, 

t m = 0.408 s 


: 63.1 V 

This maximum is larger than that obtained in the overdamped case and 
is a result of the smaller losses that occur in the larger resistor; the time 
of the maximum response is slightly later than it was with overdamping. 
The settling time may also be determined by solving 


= 420t.e~ 2A5 '' 

for t s (by trial-and-error methods), 

t a = 3.12 s 

which is a considerably smaller value than arose in the overdamped case. 
As a matter of fact, it can be shown that, for given values of L and C, 
the selection of that value of R which provides critical damping will always 
give a shorter settling time than any choice of R which produces an 
overdamped response. However, a slight improvement (reduction) in 
settling time may be obtained by a further slight increase in resistance; 

Fig. 7-4 The response «(*) = 420fer 2 - 451 of the network shown 
Fig. 7-2 with R changed to provide critical damping. 


8.57 Q , 

7H3 -^Fsfco 

i(0) = 10 A 
t)(0) - 
a = ai = -SB 
Critical damping 

J >t (s) 

210 Tne Transient Circuit 

a slightly underdamped response which will undershoot the zero axis before 
it dies out will yield the shortest settling time. 

The response curve for critical damping is drawn in Fig. 7-4; it may 
be compared with the overdamped (arjd underdamped) case by reference 
to Fig. 7-6. 

Drill Problem 

7-4 Find v(t) for each of the following cases if the damping is critical: (a) 
R = 1 VSl, L = 2 H, c(0) = 10 V, 1(0) = 10 mA; (b) L = 0.1 H, C = 10 (nF, 
u(0) = 10 V, t(0) = 10 mA; (c) fi = 20 kQ, C = 0.025 ,uF, v(0) = 10 V, i(0) = 
10 mA. 

Ans. 10e- looot (l - 900t); 10e- lm0 '(l + lOOOt); 10er looot (l + 390,000t) V 


Let us continue the process begun in the last section by increasing R once 
more. Thus, the damping coefficient a decreases while o> remains constant, 
a 2 becomes smaller than <o 2 , and the radicand appearing in the expressions 
for s t and s 2 becomes negative. This causes the response to take on quite 
a different character, but it is fortunately not necessary to return to the 
basic differential equation again. By using complex numbers, the exponen- 
tial response turns into a sinusoidal response; this response is composed 
entirely of real quantities, the complex quantities being necessary only for 
the derivation. 4 

We therefore begin with the exponential form 

v(t) = Aje* 1 ' + A 2 e" 2 ' 

*1,2 — 

— a ± Va 2 — "o 2 

and then let 

V« 2 - 

-V = 

V-i V" 2 -« 2 

/' V" 2 - a 


4 An introduction to the use of complex numbers appears in Chap. 9 and Appendix 3. At 
that time we shall emphasize the more general nature of complex quantities by identifying 
them with boldface type; no special symbolism need be adopted in these few pages. 

211 The RLC Circuit 

We now take the new radical, which is real for the underdamped case, 
and call it u d , the natural resonant frequency, 

"d = V<V - a 2 
Collecting, the response may now be written as 

v (t) = <r< rt (A 1 e»'" t + A 2 e->^" t ) 

or in the longer but equivalent form, 

v(t) = ,- {(A, + A 2 ) [ J"' Y^ ] + ^ - A 2 ) Y" 7 2 ^1) 

Two of the most important identities in the field of complex numbers, 
identities which are later proved in Appendix 3, may now be readily 
applied. The first bracket in the above equation is identically equal to 
cos co d t, and the second bracket is identically sin u d t. Hence, 

v(t) = e~"'[(A 1 + A 2 ) cos u d t + j(A 1 — A 2 ) sin a d t] 

and the multiplying factors may be assigned new symbols, 

v(t) = e-"'(B 1 cos u d t + B 2 sin u d t) (20) 

If we are dealing with the underdamped case, we have now left complex 
numbers behind. This is true since a, co d , and t are real quantities, v(t) 
itself must be a real quantity (which might be presented on an oscilloscope, 
a voltmeter, or a sheet of graph paper), and thus B 1 and B 2 are real 
quantities. Equation (20) is the desired functional form for the under- 
damped response, and its validity may be checked by direct substitution 
into the original differential equation; this exercise is left to the doubters. 
The two real constants B 1 and B 2 are again selected to fit the given initial 

Let us increase the resistance in our example from 7"\/6/2 or 8.57 
to 10.5 y2 or 14.85 £2; L and C are unchanged. Thus, 

a = 2RC 

1 =V2 


and u d = V" 2 — a2 = 2 (rad/s) 

212 Tn * Transient Circuit 

Except for the evaluation of the arbitrary constants, the response is now 

v(t) = e-^ t (B 1 cos 2t + B 2 sin Zt) 

The determination of the two constants proceeds as before. If we again 
assume that v(0) = and i(0) = 10, then B 1 must be zero. Hence, 

v(t) = B 2 e~^< sin 2t 

The derivative is 

4$- - 2B?e-^< cos It - V2B 2 e~^' sin 2t 

and at t = it becomes 

aU"™ 1- c 

* I = 2B , = ^# = 420 


v(t) = ZlOe' 1414 ' sin 2* 

Notice that, as before, this response function has an initial value of zero, 
because of the initial voltage condition we imposed, and a final value of 
zero, because the exponential term vanishes for large values of t. As t 
increases from zero through small positive values, v(t) increases as 210 sin 2t 
because the exponential term remains essentially equal to unity. But at 
a time t m , the exponential function begins to decrease more rapidly than 
sin It is increasing; so v(t) reaches a maximum v m and begins to decrease. 
We should note that t m is not the value of t for which sin 2t is a maximum, 
but must occur somewhat before sin 2* reaches its maximum value. When 
* = ir/2, v(t) is zero; for the interval 77/2 < t < it the response is negative, 
becoming zero again at t = it. Thus v(t) is an oscillatory function of time 
and crosses the time axis an infinite number of times at t = nir/2, where 
n is any positive integer. In our example, however, the response is only 
slightly underdamped and the exponential term causes the function to die 
out so rapidly that most of the zero crossings will not be evident in a sketch. 

The oscillatory nature of the response becomes more noticeable as a 
decreases. If a is zero, which corresponds to an infinitely large resistance, 
then v(t) is an undamped sinusoid which oscillates with constant amplitude. 
This is not perpetual motion; we have merely assumed an initial energy 
in the circuit and have not provided any means to dissipate this energy. 
It is transferred from its initial location in the inductor to the capacitor, 

> I (s) 

Fig. 7-5 The response v(t\ = 2\0e~ lilil sin It of the network shown 
in Fig. 7-2 with R increased to produce an underdamped response. 

then returns to the inductor, and so on, forever. Actual parallel RLC 
circuits can be made to have effective values of R so large that a natural 
undamped sinusoidal response can be maintained for years without supply- 
ing any additional energy. We can also build active networks which 
introduce a sufficient amount of energy during each oscillation of v(t) so 
that a sinusoidal response which is nearly perfect can be maintained for 
as long as we wish. This circuit is a sinusoidal oscillator, or signal generator, 
which is an important laboratory instrument. 

Returning to our specific numerical problem, differentiation locates the 
first maximum of v(t), 

the succeeding minimum, 

= -9.47 V 

at « m , = 2.05 s 

and so on. The response curve is shown in Fig. 7-5. 

The settling time may be obtained by a trial-and-error solution, and 
it turns out to be 3.88 s, a little larger than for critical damping. Problem 
15 at the end of this chapter demonstrates that the shortest settling time 
for this network results for slight underdamping. 

The overdamped, critically damped, and underdamped responses for 
this network are shown on the same graph in Fig. 7-6. A comparison of 
these three curves makes these general conclusions plausible: 

1 When the damping is changed by adjusting the size of the parallel 


>* (s) 

Fig. 7-6 Three response curves for a parallel RLC circuit for which 
u = \fi, v[0) = 0, t(0) = 10 A, and a is 3.5 (overdamped), 2.45 (criti- 
cally damped}, and 1.414 (underdamped). 

resistance, the maximum magnitude of the response is greater with 
smaller damping. 
2 The minimum settling time occurs approximately for critical 
damping; actually, the response should be slightly underdamped. 

Drill Problems 

7-5 The switch in the circuit shown in Fig. 7-7 is closed at t = 0. Find v at 
t = : (a) 0; (b) 2.5 ms; (c) 5w/3 ms. 

Ans. 0.493; 1.81; 3.00 V 

250 a 

Fig. 7-7 See Drill Prob. 7-5. 

7-6 Let the element values in the circuit of Fig. 7-2 be those of the underdamped 
example in the section above (R = 10.5 V2 Q, L = 7 H, C = % 2 F). If the 
response is: v(t) = 63e-^'(cos 2t - 3 sin 2t) V, find: (a) i R {0); (b) i c (0); (c) i(0). 

Ans. -11.12; -6.88; -4.24 A 


215 The Rlc Circuil 

We now wish to determine the natural response of a circuit model com- 
posed of an ideal resistor, an ideal inductor, and an ideal capacitor con- 
nected in series. The ideal resistor may represent a physical resistor con- 
nected into a series LC or RLC circuit, it may represent the ohmic losses 
and the losses in the ferromagnetic core of the inductor, or it may be used 
to represent all these and other energy-absorbing devices. In a special case, 
the resistance of the ideal resistor may even be exactly equal to the meas- 
ured resistance of the wire out of which the physical inductor is made. 
The series RLC circuit is the dual of the parallel RLC circuit, and this 
single fact is sufficient to make its analysis a trivial affair. Figure 7 -8a shows 
the series circuit. The fundamental integrodifferential equation is 

di 1 r' 

L-j t + Ri + -J idt-v c (t ) = 

and should be compared with the analogous equation for the parallel RLC 
circuit, drawn again in Fig. 7-8b, 

dv 1 1 r' 

C lh + R V+ L-l Vdt - iM = 

The second-order equations obtained by differentiating each of these 
equations with respect to time are also duals, 

, d 2 v , 1 dv 
dt 2 R dt ' L 

r* a V , 1 an , C _ n /oo\ 

^^JTF + "5"3T + T - u y^l 

It is apparent that our complete discussion of the parallel RLC circuit 
is directly applicable to the series RLC circuit; the initial conditions on 
capacitor voltage and inductor current are equivalent to the initial condi- 
tions on inductor current and capacitor voltage; the voltage response 

Fig. 7-8 (a) The series RLC circuit which is the dual of (b) the parallel 
RLC circuit. Element values are of course not identical in (a) and (fo). 

C I 



216 * ne Transient Circuit 

becomes a current response. It is quite possible to reread the previous four 
sections (including the drill problems) using dual language and thereby 
obtain a complete description of the series RLC circuit. 5 This process, 
however, is apt to induce a mild neurosis after the first few paragraphs 
and does not really seem to be necessary. 

A brief resume of the series circuit response is easily collected. In terms 
of the circuit shown in Fig. 7-8a, the overdamped response is 

i{t) = A^ 1 ' + A 2 e« 2i 


and thus 

H * - 2L ± V \2l) 



— — a ± V<* 2 — w o 2 

= -a ± ju d 



W = ; 

"d = V" 2 - » 2 
The form of the critically damped response is 
i(t) = e- a, (A 1 t + A 2 ) 
and the underdamped case may be written 

i(t) = e- a '(B 1 cos u d t + B 2 sin u d t) 

It is evident that if we work in terms of the parameters «, <o , and u d 
the mathematical forms of the responses for the dual situations are identi- 
cal. An increase in a in either the series or parallel circuit, while keeping 
o) constant, tends toward an overdamped response. The only caution that 
we need exert is in the computation of a, which is 1/2BC for the parallel 
circuit and R/2L for the series circuit; thus, a is increased by increasing 
the series resistance or decreasing the parallel resistance. 

5 In fact, during the writing of this text, the authors had originally written these first sections 
to describe the series RLC circuit. But, after deciding that it would be better to present 
the analysis of the more practical parallel RLC circuit first, it was easy to go back to the 
original writing and replace it with its dual. The numerical values of several of the elements 
were also scaled, a process described later in Chap. 14. 

217 Ths Rt C Circuit 

As a numerical example, let us consider a series RLC circuit in which 
L=lH,B=2ld!,C= % 01 ixF, i(0) = 2 mA, and v^O) = 2 V. We find 
that a is 1000 and co is 20.02 X 10 3 , and thus an underdamped response 
is indicated; we therefore calculate the value of co d and obtain 2 X 10 4 . 
Except for the evaluation of the two arbitrary constants, the response is 
now known: 

i(t) = e" 10001 ^ cos 2 X 10 4 t + B 2 sin 2 X 10 4 () 

By applying the initial value of the current, we find 

8, = 2X 10- 3 
and thus 

i(t) = e - 10001(2 X 10~ 3 cos 2 X 10 4 f + B 2 sin 2 X 10 4 t) 

The remaining initial condition must be applied to the derivative; thus, 

it = e -iooot(_ 40 sin 2 x 10 4 f + 2 x 10 4 B 2 cos 2 X 10H 

- 2 cos 2 X 10 4 t - 1000B 2 sin 2 X 10 4 () 


= 2 X 10 4 B 2 2 = " t(0) = 

% (0) - Ri(0) 

_ 2 - 2 X 10 3 (2 X 10- 3 ) _ 


B 2 = 

Fig. 7-9 The current response in an underdamped series RLC circuit 
for which a = 1000 s"\ w d = 2 X 10 4 s" 1 , i(0) = 2 mA, v^Q) = 2 V. 
The graphical construction is simplified by drawing in the envelope, shown 
as a pair of broken lines. 
i(t) JmA) 

-^ ( (ms) 

218 The Trans ' en » Circuit 

The desired response is, therefore, 

i(t) = 2 X 10- 3 e- 1000J cos 2 X 10 4 f A 

This response is more oscillatory, or shows less damping, than any we 
have considered up to this time, and the direct calculation of enough points 
to graph a smooth response curve is a tedious undertaking. A good sketch 
may be made by first drawing in the two exponential envelopes, 

2 X 10- 3 e- 1000 ' and -2 X 10" 3 e~ 

as shown by the broken lines in 

Fig. 7-9. The location of the quarter-cycle points of the sinusoidal wave 
at 2 X WH = 0, it/2, it, etc., or t = 0.07854A: ms, k = 0, 1, 2, . . . , by 
light marks on the time axis then permits the oscillatory curve to be 
sketched in quickly. 

Drill Problems 

7-7 Note that the current source in the circuit of Fig. 7-10 goes to zero at £ = 0, 
and find i(0 + ) and i'(0+) if R = : (a) 500 52; (b) 400 52; (c) 320 52. 

Ans. Each is 10 mA, A/s 



mA V^V 

Fig. 7-10 See Drill Probs. 7-7 and 7-8. 

7-8 Find i(t) at t = 50 ms for the circuit of Fig. 7-10 if R = : (a) 500 U; (b) 
400 52; (c) 320 52. 

Ans. 7.09; 7.36; 7.64 mA 


We must now consider those RLC circuits in which dc sources are switched 
into the network and produce forced responses that do not vanish as time 
becomes infinite. The general solution is obtained by the same procedure 
that was followed in RL and RC circuits; the forced response is determined 
completely, the natural response is obtained as a suitable functional form 
containing the appropriate number of arbitrary constants, the complete 
response is written as the sum of the forced and the natural responses, and 
the initial conditions are then determined and applied to the complete 

219 The R1C Circuit 

response to find the values of the constants. It is this last step which is 
quite frequently the most troublesome to students. Consequently, although 
the determination of the initial conditions is basically no different for a 
circuit containing dc sources than it is for the source-free circuits which 
we have already covered in some detail, this topic will receive particular 
emphasis in the examples that follow. 

Most of the confusion in determining and applying the initial conditions 
arises for the simple reason that we do not have laid down for us a rigorous 
set of rules to follow. At some point in each analysis there usually arises 
a situation in which some thinking is involved that is more or less unique 
to that particular problem. This originality and flexibility of thought, as 
simple as it is to achieve after several problems' worth of practice, is the 
source of the difficulty. 

The complete response (arbitrarily assumed to be a voltage response) 
of a second-order system consists of a forced response, which is a constant 
for dc excitation, 

v,(t) = V, 

and a natural response 


v n (t) = Ae 81 ' + Be 82 ' 

v(t) = V f + Ae 81 ' + Be 82 ' 

We shall now assume that s v s 2 , and V f have already been determined from 
the circuit and the given forcing functions; A and B remain to be found. 
The last equation shows the functional interdependence of A, B, v, and 
t, and substitution of the known value of v at t = + thus provides us with 
a single equation relating A and B. Another relationship between A and 
B is necessary, and this is normally obtained by taking the derivative of 
the response, 

^- = + Sl Ae*i< + s 2 Be> 2 * 

and inserting in it the known value of dv/dt at t = 0+. There is no reason 
that this process cannot be continued; a second derivative might be taken, 
and a third relationship between A and B will then result if the value of 
d 2 v/dt 2 at t = + is used. This value is not usually known, however, in 
a second-order system; as a matter of fact, we are much more likely to 
use this method to find the initial value of the second derivative if we should 
need it. We thus have only two equations relating A and B, and these may 
be solved simultaneously to evaluate the two constants. 


5 A 

Fig. 7-1 1 An RLC circuit which is used to illustrate several procedures 
by which the initial conditions may be obtained. The desired response is 
nominally taken to be v^t). 

The only remaining problem is that of determining the values of v and 
dv/dt at t = + . Since i c = C dv c /dt, we should recognize the relationship 
between the initial value of dv/dt and the initial value of some capacitor 
current. If we can establish a value for this initial capacitor current, then 
we shall automatically establish the value of dv/dt. Students are usually 
able to get v(0 + ) very easily, but are inclined to stumble a bit in finding 
the initial value of dv/dt. If we had selected a current as our response, 
then the initial value of di/dt must be intimately related to the initial value 
of some inductor voltage. 

Let us illustrate the procedure by the careful analysis of the circuit 
shown in Fig. 7-11. To simplify the analysis, an unrealistically large capaci- 
tor is used again. Our object is to find the value of each current and voltage 
at both t = 0~ and t = + ; with these quantities known, the required 
derivatives may be easily calculated. We shall employ a logical step-by-step 
method first. 

At t — 0~, only the right-hand current source is active. Moreover, the 
circuit is assumed to have been in this state forever, and all currents and 
voltages are constant. In other words, a steady-state condition has been 
reached and the resultant forced response has the form of the forcing 
function, its integral, and its derivatives. The integral of the forcing 
function, a linearly increasing function of time, is not present in this circuit, 
for it can occur only when a constant current is forced through a capacitor 
or a constant voltage is maintained across an inductor. This situation should 
not normally be present because the capacitor voltage or inductor current 
would assume an unrealistic infinite value at t = 0~. Continuing, then, a 
constant current through the inductor requires zero voltage across it, 

v L (0~) = 

and a constant voltage across the capacitor requires zero current through 

%(0-) = 


221 The R1C Circuit 

We then apply Kirchhoff's current law to the right node to obtain 

i s (0~) = -5 A 
which also yields 

%(0")= -150 V 

We may now use Kirchhoff's voltage law around the central mesh, finding 

v c (0-) = 150 V 
while Kirchhoff's current law enables us to find the inductor current, 

i L (0") = 5 A 

Although the derivatives at t — 0~ are of little interest to us, it is evident 
that they are all zero. 

Now let time increase an incremental amount. During the interval from 
t — 0~ to t = + , the left-hand current source becomes active and most 
of the voltage and current values at t — 0~ will change abruptly. However, 
we should begin by focusing our attention on those quantities which cannot 
change, inductor current and capacitor voltage. Both of these must remain 
constant during the switching interval. Thus, 

i t (0+) = 5 A and o c (0+) = 150 V 

Since two currents are now known at the left node, we next obtain 6 

i R (0 + ) = -1 A and v R (0+) = -30 V 

ip(0 + ) = 4 A and v L (0 + ) = 120 V 

There remain six derivatives which might be evaluated, although not all 
are needed to evaluate the two arbitrary constants. The procedure must 
begin with the energy-storage elements by the direct application of their 
defining equations. For the inductor, 

% = ^ 

L dt 

6 This current is the only one of the four remaining quantities which can be obtained in 
one step. In more complicated circuits, it is quite possible that none of the remaining initial 
values can be obtained with a single step; either circuit equations must then be written 
or a simpler equivalent resistive circuit must be drawn which can be analyzed by writing 
simultaneous equations. This latter method will be described shortly. 

222 T 1 * 6 Transient Circuit 

and, specifically, 


*| -"f +) -40 A/s 
dt | (=0+ L 


dc | = «° + ) = 108 v/s 

The other four derivatives may be determined by realizing that KirchhofF s 
current and voltage laws are both satisfied by the derivatives also. For 
example, at the left node, 

and thus 

and, therefore, 

4-i L -i R = f > 

dt dt 

^M = -40 A/s 

at I ,_ n+ 

Now let us turn to a slightly different method by which all these 
currents, voltages, and derivatives may be evaluated at t = 0~ and t = + . 
We shall construct two equivalent circuits, one which is valid for the 
steady-state condition reached at t = 0~ and a second which is valid during 
the switching interval. The discussion which follows relies on some of the 
reasoning we did above and, for that reason, appears shorter than it would 
be if it were presented first. 

Prior to the switching operation, only direct currents and voltages exist 
in the circuit, and the inductor may therefore be replaced by a short circuit, 
its dc equivalent, while the capacitor is replaced by an open circuit. 
Redrawn in this manner, the circuit of Fig. 7-11 appears as shown in Fig. 
7-12a. The three voltages and three currents at * = 0~ are now easily found 
by resistive circuit-analysis methods; the numerical values are the same 
as those found previously. 

We now turn to the problem of drawing an equivalent circuit which 
will assist us in determining the several voltages and currents at t = + . 
Each capacitor voltage and each inductor current must remain constant 
during the switching interval. These conditions may be ensured by replac- 
ing the inductor by a current source and the capacitor by a voltage source. 


(a) (6) 

Fig. 7-12 (a) A simple circuit which is the equivalent of the circuit of 
Fig. 7-11 for t = 0~. [b\ Another equivalent of the circuit of Fig. 7-11, 
valid during the switching interval, t = 0~ to t = + . 


Each source serves to maintain the necessary response constant during the 
discontinuity. The equivalent circuit of Fig. 7-12fo results; it should be 
noted that this circuit is a true equivalent at t = 0~ since it possesses the 
same currents and voltages as the simple equivalent of Fig. 7- 12a. It is 
also a true equivalent at t = + since the step-current source appears as 
a function of time and not merely as A or 4 A. 

The voltages and currents at t = 0+ are obtained by letting 4u(i) — 4 A 
and solving the dc circuit which results. The solution is not difficult, but 
the relatively large number of sources present in the network does produce 
a somewhat strange sight. However, problems of this type were solved' 
in Chap. 3, and nothing new is involved. The six responses at t — + must 
agree with those found by the previous method. 

Before leaving this problem of the determination of the necessary initial 
values, it should be pointed out that at least one other powerful method 
of determining them has been omitted; we could have written general nodal 
or loop equations for the original circuit. Then, the substitution of the 
known zero values of inductor voltage and capacitor current at t = 0~ 
would uncover several other response values at t = 0~ and enable the 
remainder to be found easily. A similar analysis at t — + must then be 
made. This is an important method, and it becomes a necessary one in 
more complicated circuits which cannot be analyzed by the simpler step- 
by-step procedures we have followed. However, we must leave a few topics 
to be covered at the time operational methods of circuit analysis are 
introduced later. 

Now let us briefly complete the determination of the response v^t) for 
the original circuit of Fig. 7-11. With both sources dead, the circuit appears 
as a series RLC circuit and s 1 and s 2 are easily found to be —1 and —9, 
respectively. The forced response may be found by inspection or, if neces- 
sary, by drawing the dc equivalent, which is similar to Fig. 7-12a, with 
the addition of a 4-A current source. The forced response is 150 V. Thus, 


v c (t) = 150 + Ae~' + Be" 9 ' 
u c (0+) = 150 = 150 + A + B 

224 "•• Trantienl Circuit 




dv c 

dv c 

= -Ae- 

= 108 


-A - 9B 

A = 13.5 £ = - 13.5 

v c (t) = 150 + 13.5(e- ( - e~ st ) 

Drill Problems 

7-9 For the circuit shown in Fig. 7-13, determine values at t = and t = + 
for: (a) t^; (h) t> 2 ; (c) v 3 . 

Ans. -0.4, -0.4; -0.4, -0.4; 0, 1.2 V 

120 n 

Fig. 7-13 See Drill Probs. 7-9 to 7-11. 

7-10 For the circuit of Fig. 7-13, find values at t = 0" and t = 0+ for: (a) dvjdt; 
(b) dv 2 /dt; (c) dv 3 /dt. 

Ans. 0, -176; 0, 64; 0, 96 V/s 

7-1 1 For the circuit of Fig. 7-13, for t > 0, find: (a) v^t); (b) v 2 (t); (c) v 3 (t). 

Ans. 0.4 - 0.533e- 40 ' - 0.267e- 160 <; 0.133e- 40 ' + 1.067e- leot ; 

0.4 - 0.267e- 40 ' - 0.533e- 160( V 


D 1 A parallel circuit is comprised of the elements, L = 10 H, R = 320 Q, 
C = 12 % fiF. The initial value of the capacitor voltage is v^O) = — 160 V and 
the initial value of the capacitor current is i c (0 + ) = 0.7 A, where i c and v c are 
related by the passive sign convention, (a) Find the initial energy storage in the 
inductor and capacitor, (b) At what value of t is x> c — 0? (c) At what value of 
t is v c a positive maximum? 

225 Tho R1C Circui * 

D 2 (a) The circuit shown on the response curve of Fig. 7-3 is modified by increasing 
the size of the inductor to 140 %3 H. If the initial conditions remain unchanged, 
find and sketch v(t); compare with the response of the original circuit, (b) What 
will the response become as L approaches infinity? 

D 3 The voltage across a source-free parallel RLC circuit is v c (t) = 10e~ 1000 ' — 
5 e -4000( v for (> 0. If the energy stored in the capacitor at t = is 100 fij, find 
R, L, C, v c (0), and i t (0). 

□ 4 The circuit shown in Fig. 7-14 is source-free for t > 0. Find v(t). 

25 n 

50u(-()v(+) 16juF5StJ<(> 

Fig. 7-14 See Probs. 4 and 6. 

□ 5 After being open for a long time, the switch in the circuit of Fig. 7-15 is closed 
at t = 0. Find i(t) for t > 0. 

1 A 

Fig. 7-15 See Probs. 5 and 10. 

D 6 (a) What value of resistance must be placed in series with the 25-il resistor 
of Fig. 7-14 to create critical damping? (b) With this resistor in place, find v(t) 
for t > 0. 

□ 7 A certain parallel RLC circuit has an exponential damping coefficient of 
500 s -1 and a resonant frequency of 400 rad/s. It is found experimentally that 
adding a 2-juF capacitor in parallel with the circuit produces critical damping. 
If the voltage across the critically damped circuit is v(t) and v(0) = 20 V while 
o'(0+) = 2000 V/s, find t>(t) for t > 0. 

□ 8 For a critically damped parallel RLC circuit in which vJO) = 0, show that 
v c reaches a maximum at t m = \/a and that the total energy stored in the circuit 
then is 5e -2 times the energy stored in the inductor at t = 0. 

□ 9 The natural response of a source-free parallel RLC circuit for t > is v(t) = 
100e~ 600t cos 400t V. If the initial energy stored in the capacitor is % J, find R, 
L, C, and the initial inductor current. 

226 Tne Transient Circuit 

□ 10 Let the capacitance in Fig. 7-15 be changed to 13 /iF. The switch is now 
left open for a long time and is then closed at t = 0. Find i(t) for ( > 0. 

Dll The switch in the circuit of Fig. 7-16 lias been closed during a laboratory 
experiment. Seeing a maximum source voltage of only 10 V in the circuit, student 
D carelessly lets his hands roam all over it; in particular, across the inductor at 
t = just as his newest enemy opens the switch. What is the maximum voltage 
to which he will be subjected? Sketch v L (t) vs. t. 

t = 

5f: 100 /iF 

Fig. 7-16 See Prob. 11. 

□ 12 A parallel RLC circuit consists of a 100-pF capacitor, a 5-kfi resistor, and 
a 2-mH inductor. If the capacitor voltage and inductor current (as sensed in Fig. 
7-2) are 2 V and 1 mA, respectively, at t = 0, find i c (t) for t > 0. 

□ 1 3 A parallel RLC circuit contains a 750-J2 resistor, a 10 / 3 -i*F capacitor, and an 
inductor L. Let the initial stored energies be u>p(0) = and u> L (0) = 0.05 J. Find 
the maximum magnitude of the capacitor voltage, the time t m at which it occurs, 
and the settling time t a if L = : (a) 10 H; (b) 7.5 H; (c) 6 H. 

□ 14 A series RLC circuit contains a 2-(*F capacitor, a %-H inductor, and a 
2600-SJ resistor. If the inductor current and voltage (v L = L di L /dt) at * = 
are v L = 30 V, i L = 50 mA, find i L (t) for t > 0. 

□ 1 5 The resistance of the underdamped circuit shown in Fig. 7-5 is changed from 
14.85 Q to 10.5 U. After finding the response v(t), determine: (a) the time t ml 
and voltage v ml for the first maximum; (b) the time t 01 for the first zero crossing; 
(c) the time t m2 and voltage u m2 for the first minimum; and (d) the settling 
time t„. 

□ 16 The current circulating in a series RLC circuit is i = 20e~ 1000 ' — 
lOg-40001 m A. Let the initial energy storage in the inductor be 0.2 mj. Determine 
fi, L, C, tJc(0), and iJO). 

□ 17 Find the current i(t) for * > in the circuit shown in Fig. 7-17. 

□ 1 8 It is desired to modify the circuit of Fig. 7-17 to produce critical damping 
by placing a resistance R r in parallel with the resistor already present, (a) Find 
R x . (b) Find i(t) for the critically damped circuit. 


mA V_V 

/fT^ 100 u(-t) 

Fig. 7-17 See Probs. 17 and 18. 

D 1 9 A source-free series RLC circuit has the current, i(t) = 20e~ 900 ' cos 600t mA, 
established in it for t > 0. If the series resistance is 90 S2, find L, C, and the initial 
energy stored in the capacitor and inductor. 

D 20 After being closed for 1 s, the switch in the circuit of Fig. 7-18 is opened 
at t = 0. Find i^t) for all t. 

24 V 


1 mH; 








Fig. 7-18 See Prob. 20. 

□ 21 The circuit of Fig. 7-19 has been in the configuration shown for a long time. 
At t = 0, the 100-S2 resistor is connected into the circuit as the switch opens. 
Find i(t) for all r. 


36 mA (^ 

Fig. 7-19 See Probs. 21 and 22. 

□ 22 Refer to Fig. 7-19 and change the time of the switch opening to ( = — oo 
and let the source become 36 + 36u(t) mA. Find i(t) for all t. 

□ 23 Find i L (t) for all t for the circuit shown in Fig. 7-20. 


-8 + 12«(«)/+N 

lKt> 4mH< 

0.003 nF 

Fig. 7-20 See Prob. 23. 

D 24 Find v x (t) for « < and £ > in the circuit shown in Fig. 7-21. To what 
value must the voltage source be changed in order that t^(0~) = — 1> 1 (0 + )? 

1 A 



1 H 

•i n 


u(f) V 
Fig. 7-21 See Prob. 24. 

=t=l F 

□ 25 Find and sketch v B (t) for the circuit of Fig. 7-22. 

n^v^f — 

© p ih w t 3v 

3 V 

Fig. 7-22 See Prob. 25. 

D 26 Write the single equation required to describe the circuit of Fig. 7-23, using 
i c as the variable. By comparing this equation with the basic equations for the 
series and parallel RLC circuit, determine equivalent values for H, L, and C. 
Find i c (t) for t > 0. 

Fig. 7-23 See Prob. 26. 


s kn 







: Chapter Eight 
The Sinusoidal 
Forcing Function 






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234 Sinusoidal Analysis 

of these circuits by adding the natural response, which is characteristic of 
the circuit and not of the forcing function, to the forced response produced 
by dc forcing functions, the only forced response with which we are 
familiar. We are therefore now in a position where our mastery of the 
natural response is greater than our knowledge of the forced response. 

In this third part of our study we shall extend our knowledge of the 
forced response by considering the sinusoidal forcing function. 

Why should we select the sinusoidal forcing function as the second 
functional form to study? Why not the linear function, the exponential 
function, or a modified Bessel function of the second kind? There are many 
reasons for the choice of the sinusoid, and any one of them would probably 
be sufficient to lead us in this direction. 

One of these reasons is apparent from the results of the preceding 
chapter; the natural response of an underdamped second-order system is 
a damped sinusoid, and if no losses are present it is a pure sinusoid. The 
sinusoid thus appears naturally (as does the negative exponential). Indeed, 
Nature in general seems to have a decidedly sinusoidal character; the 
motion of a pendulum, the bouncing of a ball, the vibration of a guitar 
string, the political atmosphere in any country, and the ripples on the 
surface of a stein of chocolate milk will always display a reasonably sinus- 
oidal character. 

Perhaps it was observations of these natural phenomena that led the 
great French mathematician Fourier to his discovery of the important 
analytical method embodied in the Fourier theorem. In Chap. 17 we shall 
see that this theorem enables us to represent most of the useful mathe- 
matical functions of time which repeat themselves / times a second by 
the sum of an infinite number of sinusoidal time functions with frequencies 
that are integral multiples of f ; the given periodic function f(t) can also 
be approximated as closely as we wish by the sum of a finite number of 
such terms, even though the graph of f(t) might look very nonsinusoidal. 
This decomposition of a periodic forcing function into a number of appro- 
priately chosen sinusoidal forcing functions is a very powerful analytical 
.method, for it enables us to superpose the partial responses produced in 
any linear circuit by each sinusoidal component in order to obtain the 
desired response caused by the given periodic forcing function. Thus, 
another reason for studying the response to a sinusoidal forcing function 
is found in the dependence of other forcing functions on sinusoidal analysis. 

A third reason is found in an important mathematical property of the 
sinusoidal function. Its derivatives and integrals are also all sinusoids. 1 
Since the forced response takes on the form of the forcing function, its 
integral, and its derivatives, the sinusoidal forcing function will produce 

1 We are using the term "sinusoid" collectively here to include cosinusoidal functions of time 
also. After all, a cosine function can be written as a sine function if the angle is increased 
by 90°. 

235 * ne Sinusoidal Forcing Function 

a sinusoidal forced response throughout a linear circuit. The sinusoidal 
forcing function thus allows a much easier mathematical analysis than does 
almost every other forcing function. 

Finally, the sinusoidal forcing function has important practical appli- 
cations. It is an easy function to generate and is the waveform used 
predominantly throughout the electric power industry; and every electrical 
laboratory contains a number of sinusoidal generators which operate 
throughout a tremendous range of useful frequencies. 

Drill Problem 

8-1 The Fourier theorem, which we shall study in Chap. 17, shows that 
the periodic triangular waveform v x (t), shown in Fig. 8-1, and the infinite sum of 
cosine terms, 

ITt 1 

+ cos— + -^ COS 

3 + 5 2 3 

+ W 

are equal. Determine the ratio of v 1 to v 2 at t = 6 s if v 2 is approximated by 
only: (a) two terms of the infinite series: (b) four terms of the infinite series; (c) 
six terms of the infinite series. 

Ans. 0.858; 0.950; 0.970 


> t(») 

Fig. 8-1 See Drill Prob. 8-1 . 


In this section we shall define the trigonometric nomenclature which is 
used to describe sinusoidal (or cosinusoidal) functions. The definitions 
should be familiar to most of us, and if we remember a little trigonometry, 
the section can be read over very rapidly. 

> Ut (rad) 


» t (s) 

Fig. 8-2 The sinusoidal function v(t) — V m sin u>t is plotted versus ait in 
(a) and versus t in (fe). 

Let us consider a sinusoidally varying voltage 

v(t) = V m sin w( 

shown graphically in Fig. 8-2a and b. The amplitude of the sine wave 
is V m , and the argument is co*. The radian frequency or angular frequency 
is co. In Fig. 8-2a, sin ait is plotted as a function of the argument cot, and 
the periodic nature of the sine wave is evident. The function repeats itself 
every 2tt radians, and its period is therefore 2tt radians. In Fig. 8-2fo, sin oit 
is plotted as a function of t and the period is now T. The period may also 
be expressed in degrees, or occasionally in other units such as centimeters 
or inches. A sine wave having a period T must execute l/T periods each 
second; its frequency f is l/T hertz, abbreviated Hz. Thus, one hertz is 
identical to one cycle per second, a term whose use is now discouraged 
because so many people incorrectly used "cycle" for "cycle per second." 

J T 


237 Th* Sinusoidal Forcing Function 

and since 

uT = 2it 

we obtain the common relationship between frequency and radian fre- 

<o = 2irf 

A more general form of the sinusoid 

v(t) = V m sin (ut + 6) 


includes a phase angle 8 in its argument (ut + 8). Equation (1) is plotted 
in Fig. 8-3 as a function of ut, and the phase angle appears as the number 
of radians by which the original sine wave, shown as a broken line in the 
sketch, is shifted to the left, or earlier in time. Since corresponding points 
on the sinusoid V m sin (ut + 8) occur 8 rad, or 0/u s, earlier, we say that 
V m sin (ut + 0) leads V m sin ut by rad. Conversely, it is correct to describe 
sin ut as lagging sin (ut + 8) by 8 rad, as leading sin (ut + 8) by — 8 rad, 
or as leading sin (ut — 6) by rad. 

In electrical engineering, the phase angle is commonly given in degrees, 
rather than radians, and no confusion will arise if the degree symbol is 
always used. Thus, instead of writing 

we customarily use 

v = 100 sin (2wl000t - |-| 

t; = 100 sin (2wl000i - 30°) 

Two sinusoidal waves that are to be compared in phase must both be.written 
as sine waves, or both as cosine waves; both waves must be written with 

Fig. 8-3 The sine wave V m sin [ut + 8) leads V" m sin at by 6 rad. 

238 Sinusoidal Analysis 

positive amplitudes; and each must be of the same frequency. It is also 
evident that multiples of 360° may be added to or subtracted from the 
argument of any sinusoidal function without changing the value of the 
function. Hence, we may say that 

»i = v »i «n (5* - 30°) 

v 2 = V m2 cos (5* +10°) 

= V m2 sin (5* + 90° + 10°) 

= V m2 sin (5t + 100°) 

by 130°, or it is also correct to say that v 1 leads u 2 by 230°, since v 2 may 
be written as 

c 2 = V m2 sin (5t - 260°) 

V ml and V m2 are each assumed to be positive quantities. Normally, the 
difference in phase between two sinusoids is expressed by that angle which 
is less than or equal to 180° in magnitude. 

The concept of a leading or lagging relationship between two sinusoids 
will be used extensively, and the relationship should be recognizable both 
mathematically and graphically. 

Drill Problems 

8-2 Find the angle by which u 2 leads v x if v 1 = 4 cos (1000* — 40°) and t> 2 = : 
(a) 3 sin (lOOOf + 40°); (b) -2 cos (1000« - 120°); (c) 5 sin (1000* - 180°). 

Ans. -10°; 100°; 130° 

8-3 Express each of the following in the form of A cos (at + 6) by specifying 
A and 6: (a) 6 cos ut — 4.5 sin <of; (b) 4 cos (<ot — 45°) + 3 sin (ut — 45°); (c) 
5 cos (<ot — 36.87°) + 2 cos ut — 6 sin at. 

Ans. 5, -81.9°; 6.71, 26.6°; 7.5, 36.9° 


Now that we are familiar with the mathematical characteristics of sinusoids 
and can describe and compare them intelligently, we are ready to apply 
a sinusoidal forcing function to a simple circuit and to obtain the forced 
response. We shall first write the differential equation which applies to 

239 Th* Sinusoidal Forcing Function 

the given circuit. The complete solution of this equation is composed of 
two parts, the complementary solution (which we refer to as the natural 
response) and the particular integral (or forced response). The natural 
response is independent of the mathematical form of the forcing function 
and depends only upon the type of circuit, the element values, and the 
initial conditions. We find it by setting all the forcing functions equal to 
zero, thus reducing the equation to the simpler linear homogeneous differ- 
ential equation. We have already determined the natural response of many 
RL, RC, and RLC circuits. 

The forced response has the mathematical form of the forcing function, 
plus all its derivatives and its first integral. From this knowledge, it is 
apparent that one of the methods by which the forced response may be 
found is by assuming a solution composed of such a sum of functions, where 
each function has an unknown amplitude to be determined by direct 
substitution into the differential equation. This is a lengthy method, but 
it is the one which we shall use in this chapter to introduce sinusoidal 
analysis because it involves a minimum of new concepts. If the simpler 
method to be described in the following chapters were not available, circuit 
analysis would be an impractical, useless art. 

The term steady-state response is used synonymously with forced 
response, and the circuits we are about to analyze are commonly said to 
be in the "sinusoidal steady state." Unfortunately, steady state carries the 
connotation of "not changing with time" in the minds of many students. 
This is true for dc forcing functions, but the sinusoidal steady-state response 
is definitely changing with time. The steady state simply refers to the 
condition which is reached after the transient or natural response has died 

Now let us consider the series RL circuit shown in Fig. 8-4. The 
sinusoidal source voltage v s = V m cos tot has been switched into the circuit 
at some remote time in the past, and the natural response has died out 
completely. We seek the forced response, or steady-state response, and 
it must satisfy the differential equation 

L^r + Ri = V™ cos cot 

Fig. 8-4 A series RL circuit for which fhe forced response is desired. 

240 Sinusoidal Analysis 

The functional form of the forced response is next obtained by integration 
and repeated differentiation of the forcing function. Only two different 
forms are obtained, sin cot and cos cot. The forced response must therefore 
have the general form 

i(t) = I x cos cot + I 2 sin cot 

where I 1 and Z 2 are rea l constants whose values depend upon V m , R, L, 
and co. No constant or exponential function can be present. Substituting 
the assumed form for the solution into the differential equation yields 

L( — ZjU sin cot + Z 2 co cos cot) + R(/ 1 cos cot + I 2 sin cot) = V m cos cot 

If we collect the cosine and sine terms, we obtain 

(-L/jCo + Rl 2 ) sin cot + (LI 2 u + RI X - VJ cos cot = 

This equation must be true for all values of t, and this can be achieved 
only if the factors multiplying cos cot and sin cot are each zero. Thus, 

-coU x + RI 2 = coL7 2 + RI t - V m = 

and simultaneous solution for I x and Z 2 leads to 

RV m . coLV„ 

j _ " -m j _ 

R 2 + C0 2 L 2 2 R 2 + C0 2 L 2 

Thus, the forced response is obtained, 


*(t) = -^o ^272 cos w ' + S* T7¥ sin ut ( 2 ) 

w fi 2 + co 2 L 2 R 2 + co 2 L 2 

This expression is slightly cumbersome, however, and a clearer picture 
of the response can be obtained by expressing the response as a single 
sinusoid or cosinusoid with a phase angle. Let us select the cosinusoid in 
anticipation of the method in the following chapter, 

i(t) = A cos (cot - 9) (3) 

At least two methods of obtaining the values of A and 8 should suggest 
themselves. We might substitute (3) directly into the original differential 
equation, or we could simply equate the two solutions (2) and (3). Let 
us select the latter method, since the former makes an excellent problem 
for the end of the chapter, and equate (2) and (3) after expanding the 

24 1 Th« Sinusoidal Forcing Function 

function cos (cot — 0), 

A cos 9 cos ut + A sin sin ut = 

R' + M ^ + R' + Zl* *"" 

Thus, again collecting and setting the coefficients of cos cot and sin cot equal 
to zero, we find 

A cos 8 = 

«V m 


A sin = 

«LV m 

R 2 + <c 2 L 2 " ""' " R 2 + co 2 L 2 

To find A and 9, we divide one equation by the other, 

Asjne =tan< , =i £ 
A cos fl 

and by drawing a small triangle, as shown in Fig. 8-5, we have 


A = ■ 



RV m 


VR r +^ 2 l? 

A =■ 

cosOR 2 + a 2 L 2 "' " VR 2 + oi 2 L 2 
The alternative form of the forced response therefore becomes 

»(() = 

VR 2 + « 2 L 2 

("' ~ tan_1 x) 


The electrical characteristics of the response i(t) should now be con- 
sidered. The amplitude of the response is proportional to the amplitude 
of the forcing function; if it were not, the linearity concept would have 
to be discarded. The amplitude of the response also decreases as R, L, 
or co is increased, but not proportionately. This is confirmed by the differ- 

Fig. 8-5 A right triangle displ ays the relati onship, tan = uL/R, and 
enables us to write cos 6 = R/ y/R 2 + io 2 ZA 

VH 2 + U*L 2 

242 Sinusoidal Analysis 

ential equation, for an increase in R, L, or di/dt requires a decrease in 
current amplitude if the source-voltage amplitude is not changed. The 
current is seen to lag the applied voltage by tan -1 (01L/R), an angle between 
and 90°. When <o = or L = 0, the current must be in phase with the 
voltage; since the former situation is direct current and the latter provides 
a resistive circuit, the result is expected. If R = 0, the current lags the 
voltage by 90°; then v, = L(di/dt), and the derivative- integral relationship 
between the sine and cosine indicates the validity of the 90° phase differ- 

The applied voltage and the resultant current are both plotted on the 
same ut axis in Fig. 8-6, but arbitrary current and voltage ordinates are 
assumed. The fact that the current lags the voltage in this simple RL circuit 
is now visually apparent. We shall later be able to show easily that this 
result is typical for all inductive circuits, that is, circuits composed only 
of inductors and resistors. The phase difference between the current and 
voltage depends upon the ratio of the quantity uL to R. We call coL the 
inductive reactance of the inductor; it is measured in ohms, and it is a 
measure of the opposition which is offered by the inductor to the passage 
of a sinusoidal current. Much more will be said about reactance in the 
following chapter. 

The method by which we have found the sinusoidal steady-state re- 
sponse for this simple series RL circuit has not been a trivial problem. 
We might think of the analytical complications as arising through the 
presence of the inductor; if both the passive elements had been resistors, 
the analysis would have been ridiculously easy, even with the sinusoidal 
forcing function present. The reason the analysis would be so easy results 
from the simple voltage-current relationship specified by Ohm's law. The 
voltage-current relationship for an inductor is not as simple, however; 
instead of solving an algebraic equation, we were faced with a non- 
homogeneous differential equation. It would be quite impractical to ana- 
lyze every circuit by the method described above, and in the following 
chapter we shall therefore take steps to simplify the analysis. Our result 

Fig. 8-6 The applied sinusoidal forcing function (solid) and the resultant 
sinusoidal current response (broken) of the series RL circuit shown in Fig. 8-4. 

24-3 The Sinusoidal Forcing Function 

will be an algebraic relationship between sinusoidal current and sinusoidal 
voltage for inductors and capacitors as well as resistors, and we shall be 
able to produce a set of algebraic equations for a circuit of any complexity. 
The constants and the variables in the algebraic equations will be complex 
numbers rather than real numbers, but the analysis of any circuit in the 
sinusoidal steady state becomes almost as easy as the analysis of a similar 
resistive circuit. 

Drill Problems 

8-4 Find i(t) for the circuit of Fig. 8-4 if R = 100 U, V m = 180 V, and: (a) 
a = 400 rad/s, L = 250 mH; (b) co = 200 rad/s, L = 500 mH; (c) a = 200 rad/s 
L = 50 mH. 

Arts. 127 cos (200t - 45°); 127 cos (400t - 45"); 
179 cos (200t - 5.7°) A 

8-5 A sinusoidal current source, 10 cos 1000* A, is in parallel both with a 20-fi 
resistor and the series combination of a 10-S2 resistor and a 10-mH inductor. 
Remembering the usefulness of Thevenin's theorem, find the voltage across the: 
(a) inductor; (b) 1042 resistor; (c) current source. 

Ans. 63.2 cos (lOOOt - 18.4°); 63.2 cos (lOOOt + 71.6°); 
89.4 cos (lOOOt + 26.6°) V 



□ 1 A certain sinusoidal current waveform crosses the i = axis at t = —2.1 
with i' > 0; the adjacent zero crossing occurs at t = 5.9 ms with i' < 0. (a) Find 
T, f, and w for this waveform, (b) If the current amplitude is 12 mA, write j(t) 
as a simple function of time, (c) By how many degrees does this current waveform 
lag the voltage 12 cos u>t, where voltage and current are at the same frequency? 

□ 2 Carry out the exercise threatened in the text by substituting the assumed 
current response (3), i(t) = A cos (at - 6), directly into the differential equation, 
Udi/di) + fit = V m cos ut, to show that values for A and 6 are obtained which 
agree with (4). 

□ 3 The current, i = 4 cos (200t - 45°) A, is the response produced in a series 
RL circuit by the source, v, = 150 cos (200t + 15°) V. Find R and L. 

□ 4 A voltage source, V m cos lOOf, a 20-ft resistor, and a physical coil which we 
may model with a 5-il resistor in series with a 0.5-H inductor are all in series. 
What is the ratio of the sinusoidal amplitude of the voltage across the physical 
coil to that across the 20-J2 resistor? 

244 Sinusoidal Analysis 

□ 5 The voltage source in a series RL circuit is v,(t) = 50 cos 200t + 100 sin 300t V. 
If R = 4 ft and L = 10 mH, find i(t). 

□ 6 The source voltage, v,(t) = 100 cos 20t V, is applied to a series RL circuit 
containing a 5-ft resistor and an inductor L. Find L if: (a) the amplitude of the 
current is 10 A; (b) the current waveform lags the source voltage by 30° . 

□ 7 A series circuit consists of a voltage source, v s = 20 sin 50* V, a normally open 
switch, a 642 resistor, and a 0.16-H inductor. The switch closes at t = 0. The 
desired response is the current, (a) Find the functional form of the natural 
response, (b) Find the forced response, (c) Use the initial conditions to evaluate 
the single unknown constant and determine the complete response for t > 0. (d) 
Find i at t = 40 ms. 

□ 8 In Chap. 6, the circuit of Fig. 6-12 was used as an example of the technique 
of finding the complete response to dc excitation, (a) Find i(t) if the 50u(t)-V 
source is changed to 50 cos (2*/3) V. (b) Find i(t) for t> if the 50u(J)-V source 
is changed to 50 cos (2t/3) u{t) V. 

□ 9 A current source l m cos o>t, a resistor R, and an inductor L are all in parallel. 
(a) Write the single integrodifferential equation in terms of the voltage between 
nodes, (b) Differentiate the above equation with respect to t and obtain the 
first-order linear differential equation, (c) Use the method of Sec. 8-3 to determine 
the forced response v. 

D 10 A current source I m cos ut, a resistor R, and a capacitor C are all in parallel. 
(a) Write the single linear differential equation in terms of the voltage v between 
nodes, (b) Assume a suitable general form for the forced response o, substitute into 
the above differential equation, and determine the exact form of the forced response. 

D 1 1 A voltage source 60 cos 1000* V is in series with a 2-kfi resistor and a 1-fiF 
capacitor. Find i forced . 

D 12 A 1-juF capacitor, a 10-mH inductor, and a current source 0.2 sin 8000t A are 
in parallel. The circuit is in a steady-state condition. Find the ratio of the 
amplitudes of the inductor and source currents. 

•Tlie Pfeasor Concept 


Throughout the earlier portions of our study of circuit analysis, we devoted 
our entire attention to the resistive circuit. However, we might remember 
that we were often promised that those methods which we were applying 
to resistive circuits would later prove applicable to circuits containing 
inductors and capacitors as well. In this chapter we shall lay the descriptive 
groundwork which will make this prediction come true. We shall develop 
a method for representing a sinusoidal forcing .function or a sinusoidal 
response by a complex-number symbolism called a phasor transform, or 
simply a phasor. This is nothing more than a number which, by specifying 

246 Sinotoidal Analysis 

both the magnitude and phase angle of a sinusoid, characterizes that 
sinusoid just as completely as if it were expressed as an analytical function 
of time. By working with phasors, rather than with derivatives and integrals 
of sinusoids as we did in the preceding chapter, we shall effect a truly 
remarkable simplification in the steady-state sinusoidal analysis of general 
RLC circuits. This simplification should become apparent toward the end 
of this chapter. 

The use of a mathematical transformation to simplify a problem should 
not be a new idea to us. For example, we have all used logarithms to 
simplify arithmetic multiplication and division. In order to multiply several 
numbers together, we first determined the logarithm of each of the numbers, 
or "transformed" the numbers into an alternative mathematical description. 
We might now describe that operation as obtaining the "logarithmic 
transform." We then added all the logarithms to obtain the logarithm of 
the desired product. Then, finally, we found the antilogarithm, a process 
which might be termed an inverse transformation; the antilogarithm was 
our desired answer. Our solution carried us from the domain of everyday 
numbers to the logarithmic domain, and back again. 

Other familiar examples of transform operations may be found in the 
alternative representations of a circle as a mathematical equation, as a 
geometric figure on a rectangular-coordinate plane, or merely as a set of 
three numbers, where it is understood that the first is the x-coordinate value 
of the center, the second is the y-coordinate value, and the third is the 
magnitude of the radius. Each of the three representations contains exactly 
the same information, and once the rules of the transformations are laid 
down in analytic geometry, we find no difficulty in passing from the 
algebraic domain to the geometric domain or to the "domain of the ordered 

Few other transforms with which we are familiar provide the simplifi- 
cation that can be achieved with the phasor concept. 


We are now ready to think about applying a complex forcing function (that 
is, one that has both a real and an imaginary part) to an electrical network. 1 
It may seem strange, but we shall find that the use of complex quantities 
in sinusoidal steady-state analysis leads to methods which are much simpler 
than those involving purely real quantities. We should expect a complex 
forcing function to produce a complex response; we might even suspect, 
and suspect correctly, that the real part of the forcing function will produce 

1 Appendix 3 defines the complex number and related terms, describes the arithmetic 
operations on complex numbers, and develops Euler's identity and the exponential and 
polar forms. 

v m cos iwt + e> 

l m cos (cut + <j>) 

Fig. 9-1 The sinusoidal forcing function V m cos (cot + $) produces 
steady-state sinusoidal response I m cos (wt + $). 

the real part of the response, while the imaginary portion of the forcing 
function will result in the imaginary portion of the response. Our goal 
in this section is to prove, or at least demonstrate, that these suspicions 
are correct. 

Let us first discuss the problem in rather general terms, thus indicating 
the method by which we might prove our assertions if we were to construct 
a general network and analyze it by means of a system of simultaneous 
equations. In Fig. 9-1, a sinusoidal source 

V m cos (cot + 9) 


is connected to a general network, which we shall arbitrarily assume to 
be passive in order to avoid complicating our use of the superposition 
principle later. A current response in some other branch of the network 
is to be determined. The parameters appearing in (1) are all real quantities. 
The discussion in Chap. 8 of the method whereby the response to a 
sinusoidal forcing function may be determined, through the assumption of 
a sinusoidal form with arbitrary amplitude and arbitrary phase angle, shows 
that the response may be represented by 

I m cos (cot + <t>) 


A sinusoidal forcing function always produces a sinusoidal forced response. 
Now let us change our time reference by shifting the' phase of the 
forcing function by 90° (or temporarily replacing thy t' — -n/lui). Thus, 
the forcing function 

V m cos (ut + 9 - 90°) = V m sin (cot + 9) (3) 

when applied to the same network will produce a corresponding response 

l m cos (ut + <j> - 90") = I m sin (cot + </>) (4) 

We must next depart from physical reality by applying an imaginary 
forcing function, one which cannot be applied in the laboratory but can 
be applied mathematically. 


248 Sinusoidal Analysis 

We construct an imaginary source very simply; it is only necessary to 
multiply the source, expressed by (3), by /, the imaginary operator. We 
thus apply 

jV n sm(at + e) 


What is the response? If we had doubled the source, then the principle 
of linearity would require that we double the response; multiplication of 
the forcing function by a constant k would result in the multiplication of 
the response by the same constant k. The fact that this constant is the 
imaginary operator / does not destroy this relationship, even though our 
earlier definition and discussion of linearity did not specifically include 
complex constants. It is now more realistic to conclude that it did not 
specifically exclude them, for the entire discussion is equally applicable if 
all the constants in the equations are complex. The response to the imagi- 
nary source of (5) is thus 

]l m sin (cot + <J>) 


The imaginary source and response are indicated in Fig. 9-2. 

We have applied a real source and obtained a real response; we have 
also applied an imaginary source and obtained an imaginary response. Now 
we may use the superposition theorem to find the response to that complex 
forcing function which is the sum of the real and imaginary forcing func- 
tions. The applicability of superposition, of course, is guaranteed by the 
linearity of the circuit and does not depend on the form of the forcing 
functions. Thus, the sum of the forcing functions of (1) and (5), 

V m cos (at + 6) + jV m sin (at + 8) (7) 

must therefore produce a response which is the sum of (2) and (6), 

I„ cos (at + <#>) + jl m sin (at + <t>) (8) 

The complex source and response may be represented more simply by 
applying Euler's identity. The source of (7) thus becomes 

Fig. 9-2 The imaginary sinusoidal forcing function jV m sin (cof + $) 
produces rhe imaginary sinusoidal response jl m sin [o>t + <#>). 

JV_sin (at + 6) ft 

sin (ajf + 0) 

Hot + 9) 

#<w* + *) 

Fig. 9-3 The complex forcing function V m e* u(+S) produces the complex 
response Z m e* u ' + * ) in the network of Fig. 9-1. 

v jt»t + a 


and the response of (8) is 

j e ;<ui+0> 


The complex source and response are illustrated in Fig. 9-3. 

There are several important conclusions to be drawn from this general 
example. A real, an imaginary, or a complex forcing function will produce 
a real, an imaginary, or a complex response, respectively. Moreover, a 
complex forcing function may be considered, by the use of the superposition 
theorem, as the sum of a real and an imaginary forcing function; thus the 
real part of the complex response is produced by the real part of the 
complex forcing function, while the imaginary part of the response is caused 
by the imaginary part of the complex forcing function. 

Instead of applying a real forcing function to obtain the desired real 
response, we apply a complex forcing function whose real part is the given 
real forcing function; we obtain a complex response whose real part is the 
desired real response. Through this procedure, the integrodifferential 
equations describing the steady-state response of a circuit will become 
simple algebraic equations. 

Let us try out this idea on the simple RL series circuit shown in Fig. 
9-4. The real source V m cos ut is applied; the real response Ut) is desired. 

We first construct the complex forcing function which, upon the appli- 

Fig. 9-4 A simple circuit in the sinusoidal steady state is to be analyzed by 
the application of a complex forcing function. 


°. = v m cos m ( ^, 


250 Sinusoidal Analysis 

cation of Euler's identity, yields the given real forcing function. Since 

cos ut = Re e>"' 
then the necessary complex source is 

The complex response which results is expressed in terms of an unknown 
amplitude I m and an unknown phase angle <#>, 

Writing the differential equation for this particular circuit, 
we insert our complex expressions for v s and i, 

take the indicated derivative, 

and obtain a complex algebraic equation. In order to determine the value 
of I m and 4>, we divide throughout by the common factor e* wt , 

Rl m e>* + \*UJ* = V m (11) 

factor the left side, 

l m J*(R + /<oL) = V m 


R + /«L 

and identify I m and <j> by expressing the right side of the equation in 
exponential or polar form, 

251 Tne Phaser Concept 



j Mn 

m ~ Vfi 2 + u 2 L 2 
and 4>= -tan" 1 -^- 

The complex response is given by (12). The real response t(r) may be 
obtained by reinserting the e? ut factor on both sides of (12) and taking the 
real part, easily obtained by applying Euler's omnipotent formula. Thus, 

*(*) = l m COS ("* + <t>) 

V« 2 + a 2 L? 

it at — tan -1 1 

which agrees with the response obtained for this same circuit in the previous 
chapter, Eq. (8-4). 

Although we have successfully worked a sinusoidal steady-state problem 
by applying a complex forcing function and obtaining a complex response, 
we have not taken advantage of the full power of the complex repre- 
sentation. In order to do so, we must carry the concept of the complex 
source or response one additional step and define the quantity called a 

Drill Problem 

9-1 Find the complex voltage which results when the complex current 

ClSe* 4000 '- 30 "" A is applied to: (a) a 50-H resistor; (b) a 0.01-H inductor; (c) a 
5-juF capacitor. 

Ans. 4. < Se' <4000,+60 ° ) - 6 e i<*o o o'-30°>- g e j'(4000(-i20') y 


A sinusoidal current or voltage at a given frequency is characterized by 
only two parameters, an amplitude and a phase angle. The complex 
representation of the voltage or current is also characterized by these same 
two parameters. For example, the assumed sinusoidal form of the current 
response in the example above was 

l m cos (at + <f>) 

252 Sinusoidal Analyst! 

and the corresponding representation of this current in complex form is 

Once I m and <J> are specified, the current is exactly defined. Throughout 
any linear circuit operating in the sinusoidal steady state at a single fre- 
quency <o, every current and voltage may be characterized completely by 
a knowledge of its amplitude and phase angle. Moreover, the complex 
representation of every voltage and current will contain the same factor 
e* w '. The factor is superfluous; since it is the same for every quantity, it 
contains no useful information. Of course, the value of the frequency may 
be recognized by inspecting one of these factors, but it is a lot simpler 
to write down the value of the frequency near the circuit diagram once 
and for all and avoid carrying redundant information throughout the 
solution. Thus, we could simplify the voltage source and the current 
response of the example by representing them concisely as 

V m or V m e>°- and Ij* 

These complex quantities are usually written in polar form rather than 
exponential form in order to achieve a slight additional saving of time and 
effort. Thus, the source voltage 

\ii) = V m cos cot 

we now express in complex form as 

and the current response 

i(t) = l m cos (cot + <{>) 

This abbreviated complex representation is called a phasor. Let us 
review the steps by which a real sinusoidal voltage or current is transformed 
into a phasor, and then we shall be able to define a phasor more meaning- 
fully and to assign a symbol to represent it. 

A real sinusoidal current 

'(') = 4, cos (cot + 4.) 

253 Tne P* 1050 ' Concept 

is expressed as the real part of a complex quantity by Euler's identity 

i(t) = Re (I m t? u,+ * > ) 

We then represent the current as a complex quantity by dropping the 
instruction Re, thus adding an imaginary component to the current without 
affecting the real component; further simplification is achieved by sup- 
pressing the factor e"° ( , 

I = I m ^ 
and writing the result in polar form, 

This abbreviated complex representation is the phasor representation; 
phasors are complex quantities and hence are printed in boldface type. 
Capital letters are used for the phasor representation of an electrical 
quantity because it is no longer an instantaneous function of time; the 
phasor contains only amplitude and phase information. We recognize this 
difference in viewpoint by referring to i(t) as a time-domain representation 
and terming the phasor I a frequency-domain representation. It should be 
noted that the frequency-domain expression of a current or voltage does 
not explicitly include the frequency; however, we might think of the 
frequency as being so fundamental in the frequency domain that it is 
emphasized by its omission. 2 

The process by which we change i(t) into I is called a phasor trans- 
formation from the time domain to the frequency domain. The steps in 
the time-domain to frequency-domain transformation are as follows: 

1 Given the sinusoidal function i(t) in the time domain, write i(t) as 
a cosine wave with a phase angle. For example, sin cot should be 
written as cos (cot — 90°). 

2 Express the cosine wave as the real part of a complex quantity by 
using Euler's identity. 

3 Drop Re. 

4 Suppress e* ut . 

As an example, let us transform the time-domain voltage 

v(t) = 100 cos (4O0t - 30°) 
2 Very little local mail in this country includes "U.S.A." in its address. 

25-4 Sinusoidal Analysis 

into the frequency domain. The time-domain expression is already in the 
form of a cosine wave with a phase angle, and thus we need take only 
the real part of the complex representation, 

v(t) = Re (lOOe* 400 '- 30 "') 

and drop Re and suppress e"" ( , 

V = 100 / -30" 
In a similar fashion, the time-domain current 

i(t) = 5 sin (377t + 150°) 

transforms into the phasor 

I = 5 /60° 

Before we consider the analysis of circuits in the sinusoidal steady state 
through the use of phasors, it is necessary to learn how to shift our trans- 
formation smoothly into reverse to return to the time domain from the 
frequency domain. The process is exactly the reverse of the sequence given 
above. Thus, the steps in the frequency-domain to time-domain trans- 
formation are as follows: 

1 Given the phasor current I in the frequency domain, write the 
complex expression in exponential form. 

2 Reinsert (multiply by) the factor e""". 

3 Replace the real-part operator Re. 

4 Obtain the time-domain representation by applying Euler's identity. 
The resultant cosine-wave expression may be changed to a sine 
wave, if desired, by increasing the argument by 90°. 

Thus, given the phasor voltage 

V = 115 /-45° 
we change from polar to exponential form, 

V = 115e-' 45 ° 

pass from the frequency domain to the time domain by reinserting e"° ( and 
the real-part operator, 

v(t) = Re (115e to, - 45 ° ) ) 

255 *' le P* 1050 ' Concept 

and finally invoke Euler's identity, 

v(t) = 115 cos (at - 45°) 
As a sinusoid, the answer could be written 

v(t) = 115 sin (at + 45°) 

We have been tracing the transformation process by a fairly detailed 
sequence of steps, but with a little practice it will soon be possible to make 
the transformation in either direction in a single step. Even after we have 
achieved this facility, however, it will be well to know the exact steps and 
the mathematical justification for each one. 

Before considering the methods of applying phasors in the analysis of 
the sinusoidal steady-state circuit, we may treat ourselves to a quick 
preview by returning to the example of the RL series circuit. A number 
of steps after writing the applicable differential equation, we arrived at 
(11), rewritten below, 

RI m e>* + \uhlj* = V m 

If we substitute phasors for the current, 

and the voltage 
we obtain 

fil + jaLl = V 
or (fi + juL)I = V (13) 

a complex algebraic equation in which the current and voltage are ex- 
pressed in phasor form. This equation is only slightly more complicated 
than Ohm's law for a single resistor. The next time we analyze this circuit, 
we shall begin with (13). 

Drill Problems 

9-2 Give each voltage in phasor form: (a) 20 cos (at + 40°); (b) 12 cos (ut + 360°) 
+ 10 cos (at + 70°); (c) -20 sin (at - 10°) + 20 cos (at - 50°) V. 

Ans. 15.32 + J12.86; 15.42 + J9.40; 16.33 + J4.38 V 

256 Sinusoidal Analysis 

9-3 Transform each of the following currents to the time domain: (a) 6 — ;8 A; 

(b) -8 + ;6 A; (c) -;10 A. 

Arts. 10 cos (ut - 90°); 10 cos (ut - 53.1°); 10 cos (ut + 143.1°) A 


Now that we are able to transform into and out of the frequency domain, 
we can proceed to our simplification of sinusoidal steady-state analysis by 
establishing the relationship between the phasor voltage and phasor current 
for each of the three passive elements. We shall begin with the defining 
equation for each of the elements, a time-domain relationship, and then 
let both the current and the voltage become complex quantities. After 
suppressing e 1 ^' throughout the equation, the desired relationship between 
the phasor voltage and phasor current will then become apparent. 

The resistor provides the simplest case. In the time domain, as indicated 
by Fig. 9-5a, the defining equation is 

v(t) = Ri(t) (14) 

Now let us apply the complex voltage 

V„e*" + « = V m cos (ut + 8) + jV m sin (wt + B) (15) 

and assume the complex current 

Imt p>t + = i m cos ( Wf + 0) + //m sin (ut + ^ (16) 

and obtain 

By dividing throughout by e*"' (or suppressing e*"' on both sides of the 
equation), we find 

V n e> e = RI m e^ 
or, in polar form, 

V m ll = RI m /± 

But V m /£ and I m /<t> merely represent the general voltage and current phasors 
V and I. Thus, 

V = fll (17) 



V = «I 

(a) (i) 

Fig. 9-5 A resistance R at which are present a voltage and current in: 
(<z) the time domain, v = Ri; [b] the frequency domain, V = RI. 

The voltage-current relationship in phasor form for a resistance has 
the same form as the relationship between the time-domain voltage and 
current. The defining equation in phasor form is illustrated in Fig. 9-5fo. 
The equality of the angles and <f> is apparent, and the current and voltage 
are thus in phase. 

As an example of the use of both the time-domain and frequency-domain 
relationships, let us assume a voltage of 8 cos (lOOr — 50°) V across a 4-Q 
resistor. Working in the time domain, we find that the current must be 

i(t) = ^- = 2 cos (lOOt - 50°) 

The phasor form of the same voltage is 8 /— 50" V, and therefore 

I = -5- = 2 /-50° A 

If we transform this answer back to the time domain, it is evident that 
the same expression for the current is obtained. 

It is apparent that there is no saving in time or effort when a resistive 
circuit is analyzed in the frequency domain. As a matter of fact, if it is 
necessary to transform a given time-domain source to the frequency domain 
and then translate the desired response back to the time domain, we should 
be much better off working completely in the time domain. This definitely 
does not apply to any circuit containing resistance and either inductance 
or capacitance. 

Let us now turn to the inductor. The time-domain network is shown 
in Fig. 9-6a, and the defining equation, a time-domain expression, is 

v(t) = L 



After substituting the complex voltage equation (15) and complex current 



v = L~ It V = (Oltl 


(a) (b) 

Fig. 9-6 An inductance L at which are present a voltage and current in: 
(a) the time domain, v = L di/dt; [b) the frequency domain, V = /<oLI. 

equation (16) into (18), we have 

v _Xul+«> _ r d_lj „j<ul+0)\ 

Vm6 ~ L dtV n ^ } 

Taking the indicated derivative 

V m e* <0,+8) = i«U„^" l+ * 
and suppressing e* at , 

we obtain the desired phasor relationship 

V = juLl (19) 

The time-domain differential equation (18) has become an algebraic equa- 
tion in the frequency domain. The phasor relationship is indicated in Fig. 

As an illustration of the phasor relationship, let us apply the voltage 
8 /-50° V at a frequency co = 100 rad/s to a 4-H inductor. From (19), 
the phasor current is 

or I = 0.02 / -140° A 

If we express this current in the time domain, it becomes 

i(t) = 0.02 cos (lOOt - 140°) A 

This response is also easily obtained by working entirely in the time domain; 
it is not so easily obtained if resistance or capacitance is combined with 
the inductance. 


I = >«cv 

(a) (b) 

Fig. 9-7 (a) The time-domain and [b] the frequency-domain relationship 
between capacitor current and voltage. 

The final element we must consider is the capacitor. The definition 
of capacitance, a familiar time-domain expression, is 

i(t) = C 



The equivalent expression in the frequency domain is obtained once more 
by letting v(t) and i(t) be the complex quantities of (15) and (16), taking 
the indicated derivative, suppressing e*"', and recognizing the phasors V 
and I. It is 

I = /uCV 


If the phasor voltage 8 /— 50" V is applied to a 4-F capacitor at 
a) = 100 rad/s, the phasor current is 

I = /100(4)(8 /-50°) = 3200/40° A 

The magnitude of the current is tremendous, but the assumed size of the 
capacitor is also unrealistic. If a 4-F capacitor were constructed of two 
flat plates separated 1 mm in air, each plate would have the area of about 
85,000 football fields. 3 The time-domain and frequency-domain repre- 
sentations are compared in Fig. 9- 7a and b. 

We have now obtained the V-I relationships for the three passive 
elements. Each expression is algebraic in nature. Each is also a linear 
equation, and the equations relating to inductance and capacitance bear 
a great similarity to Ohm's law. We shall use them as we use Ohm's law. 

Before we do so, we must show that phasors satisfy Kirchhoff 's two 
laws. Kirchhoff 's voltage law in the time domain is 

v i(t) + v 2 (t) + • • • + %W = 
We now use Euler's identity to replace each real voltage by the complex 

including both end zones. 


Fig. 9-8 The series RL circuit with a phasor voltage applied. 

voltage having the same real part, suppress e? ut throughout, and obtain 

V, + V 2 + ■ • • + V N = 

KirchhofFs current law is shown to hold for phasor currents by a similar 

Now let us look briefly at the series RL circuit that we have considered 
several times before. The circuit is shown in Fig. 9-8, and a phasor current 
and several phasor voltages are indicated. We may obtain the desired 
response, a time-domain current, by first finding the phasor current. The 
method is similar to that used in analyzing our first single-loop resistive 
circuit. From KirchhofFs voltage law, 

v* + v L = v s 

and the recently obtained V-I relationships for the elements 

fil + pLI = V s 
the phasor current is found in terms of the source voltage V,, 



R + juL 

Let us select a source-voltage magnitude of V m and phase angle of 0°; the 
latter merely represents the simplest possible choice of a reference. Thus, 


R + ph 

The current may be transformed to the time domain by first writing it in 
polar form, 

VR 2 + w 2 L 2 / R 

and then following the familiar sequence of steps. 

26 1 The Phaser Concept 

Drill Problems 

9-4 Given a phasor current, 30 — ;10 mA at w = 1000 rad/s, assume a passive 
sign convention and find the phasor voltage present across a: (a) 4042 resistor; 
(b) 30-mH inductor; (c) 40-juF capacitor. 

Ans. -0.25 - jO.75; 0.3 + p.9; 1.2 - p.4 V 

9-5 For each part of Drill Prob. 9-4, find the voltage across the element at 
t = 1 ms. 

Ans. -0.595; 0.496; 0.985 V 


The current-voltage relationships for the three passive elements in the 
frequency domain are 

V = RI V = koLI V = -L. 

If these equations are written as phasor-voltage phasor-current ratios 
v fi v VI 

I I ' I juC 

then we find that these ratios are simple functions of the element values, 
and frequency also, in the case of inductance and capacitance. We treat 
these ratios in the same manner we treat resistances, with the exception 
that they are complex quantities and all algebraic manipulations must be 
those appropriate for complex numbers. 

Let us define the ratio of the phasor voltage to the phasor current as 
impedance, symbolized by the letter Z. The impedance is a complex 
quantity having the dimensions of ohms. Impedance is not a phasor and 
cannot be transformed to the time domain by multiplying by e? ut and taking 
the real part. Instead, we think of an inductor L as being represented in 
the time domain by its inductance L and in the frequency domain by its 
impedance /toL. A capacitor in the time domain is a capacitance C and 
an impedance 1/juC in the frequency domain. Impedance is a part of the 
frequency domain and not a concept which is a part of the time domain. 

The validity of Kirchhoff 's two laws in the frequency domain enables 
it to be easily demonstrated that impedances may be combined in series 
and parallel by the same rules we have already established for resistances. 
For example, at to = 10 4 rad/s, a 5-mH inductor in series with a 100-/uF 
capacitor may be replaced by the single impedance which is the sum of 

262 Sinusoidal Analysis 

the individual impedances. The impedance of the inductor is 

Z t = /coL = ;50 fi 
the impedance of the capacitor is 

Z„ = -L- = -/l fi 
;wC ' 

and the impedance of the series combination is therefore 

Z eQ = ,50 - ,1 = /49 Q 

The impedance of inductors and capacitors is a function of frequency, and 
this equivalent impedance is thus applicable only at the single frequency 
at which it was calculated, co = 10,000. At to = 5000, Z eq = ;23 0. 

The parallel combination of these same two elements at co = 10 4 yields 
an impedance which is the product over the sum, 

(/50)(-,l) _ 50 
/50 - /l /49 

Z e, = £»!,= ^ = -?l-02 

At w = 5000, the parallel equivalent is — /2.17 0. 

The complex number or quantity representing impedance may be 
expressed in either polar or rectangular form. In polar form, an impedance, 
such as 100 /—60°. is described as having an impedance magnitude of 100 
and a phase angle of —60°. The same impedance in rectangular form, 
50 — ;86.6, is said to have a resistive component, or resistance, of 50 $2 and 
a reactive component, or reactance, of —86.6 0. The resistive component 
is the real part of the impedance, and the reactive component is the 
imaginary component of the impedance, including sign, but of course 
excluding the imaginary operator. It is important to note that the resistive 
component of the impedance is not necessarily equal to the resistance of 
the resistor which is present in the network. For example, a 20-0 resistance 
in series with a 5-H coil at to = 4 produces an equivalent impedance 
Z ~ 20 + /'20 0, or in polar form, 28.3 /45° U. In this case, the resistive 
component of the impedance is equal to the resistance of the series resist- 
ance because the network is a simple series network. However, if these 
same two elements are placed in parallel, the equivalent impedance is 
20(/20)/(20 + j'20), or 10 4- ;10 0. The resistive component of the im- 
pedance is now 10 0. 

No special symbol is assigned for impedance magnitude or phase angle. 
A general form for an impedance in polar form might be 

z = \z\ie_ 

'(') 1.5 kfl 

Fig. 9-9 (a) An RLC circuit for which the sinusoidal forced response i(f) 
is desired, (b) The frequency-domain equivalent of the given circuit at 
a = 3000 rad/s. 

In rectangular form, the resistive component is represented by R and the 
reactive component by X. Thus, 

Z = R + jX 

Let us now use the impedance concept to analyze an RLC circuit, shown 
in Fig. 9-9a. The circuit is shown in the time domain, and the time-domain 
response is required. However, the analysis should be carried out in the 
frequency domain. We therefore begin by drawing a frequency-domain 
circuit; the source is transformed to the frequency domain, becoming 
40 /—90° V; the response is transformed to the frequency domain, being 
represented as I; and the impedances of the inductor and capacitor, deter- 
mined at <o = 3000, are ;1 and — /2 kfl, respectively. The fre- 
quency-domain circuit is shown in Fig. 9-9fe. 

The equivalent impedance offered to the source is now calculated: 

Zeq = L5 + f xi - » = i.5 + i±4 

"« ;1 + 1 - ;2 1-/1 

15 , 2 + /11 + /1 1 + /3 

- h5 + 1 - /l 1 + ,1 ~ L5 + 2 

= 2 + /1.5 = 2.5 /36.9° kfi 

The phasor current is thus 

x \ _ 4 0/-90° 

Z eQ 2.5 /3(5.9° 

= 16 / -126.9° mA 

Upon transforming the current to the time domain, the desired response 
is obtained, 

i{t) = 16cos(3000i - 126.9°) mA 

If the capacitor current is desired, current division should be applied in 
the frequency domain. 


264 S'nutoidal Analysis 

Drill Problems 

9-6 Find the impedance at <o = 1 Mrad/s of: (a) a 2-kfi resistor in parallel with 
a 1-mH inductor; (b) the series combination of a 0.001-juF capacitor and the 
network of (a) above; (c) the parallel combination of a 0.002-juF capacitor and 
the network of (b) above. 

Am. 0.277 / -56.3° ; 0.447 / -26.6° .- 0.894 /63.4° Jtft 

9-7 In the network described in Drill Prob. 9-6, part (c), let a current source, 
20 cos 10 6 t mA, be applied and find the amplitude of the sinusoidal voltage across 
the: (a) current source; (b) 0.001-/iF capacitor; (c) 1-mH inductor. 

Ans. 5.54; 11.1; 12.4 V 


Just as conductance, the reciprocal of resistance, proved to be a useful 
quantity in the analysis of resistive circuits, so does the reciprocal of 
impedance offer some convenience in the sinusoidal steady-state analysis 
of a general RLC circuit. We define admittance Y as the ratio of phasor 
current to phasor voltage: 

Y = 

and thus 

Y =i 

The real part of the admittance is the conductance G, and the imaginary 
part of the admittance is the susceptance B. Thus, 

G + jB = ± = 

R +jX 



Equation (22) should be scrutinized carefully; it 
part of the admittance is equal to the reciprocal 
impedance or that the imaginary part of the admittance 
reciprocal of the imaginary part of the impedance, 
ance, and susceptance are all measured in mhos. 
An impedance 

Z = 1 - ;2 Q 

which might be represented, for example, by a 1- 
with a suitable capacitance, say 0.1 juF if 03 = 

not state that the real 

sf the real part of the 

is equal to the 

Admittance, conduct- 

opm resistance in series 
Mrad/s, possesses an 

265 The Photor Concept 


Y - I - 1 = * 1 + ? 2 
Z 1-/2 1 - f2 1 + /2 

= 0.2 + /0.4 

Without stopping to inspect a formal proof, it should be apparent that 
the equivalent admittance of a network consisting of a number of parallel 
branches is the sum of the admittances of the individual branches. Thus, 
the numerical value of the admittance above might be obtained from a 
conductance of 0.2 V in parallel with a positive susceptance of 0.4 U . The 
former could be represented by a 5-Q resistor and the latter by a 0.08-fiF 
capacitor at to = 5 Mrad/s , since the admittance of a capacitor is evidently 

As a check on our analysis, let us compute the impedance of this latest 
network, a 5-S2 resistor in parallel with a 0.08-juF capacitor at co = 
5 Mrad/s. The equivalent impedance is 

Sjl/juC) _ 5(-/2.5) 
5 + l//coC 5 - ;2.5 ' 

as before. These two networks represent only two of an infinite number 
of different networks which possess this same impedance and admittance 
at this frequency. They do, however, represent the only two two-element 
networks, and thus might be considered to be the two simplest networks 
having an impedance of 1 — /2 fi and an admittance of 0.2 + /0.4 at 
to = 5 X 10 6 rad/s. 

The term immittance, a combination of the words "impedance" and 
"admittance," is often used as a general term for both impedance and 
admittance. For example, it is evident that a knowledge of the phasor 
voltage across a known immittance enables the current through the immit- 
tance to be calculated. 

Drill Problems 

9-8 At 2000 rad/s, find the admittance of: (a) a 5-fi resistor in series with a 
100-(tF capacitor; (b) the parallel combination of a 2.5-mH inductor and the 
network of (a) above; (c) the series combination of a 100-/iF capacitor and the 
network of (b) above. 

Arts. 0.1 - jO.l; 0.1 + jO.l; 0.2 W 

9-9 Find the input admittance of the network shown in Fig. 9-10 at w = : (a) 
5000 rad/s; (b) 10,000 rad/s; (c) 20,000 rad/s. 

Ans. 0.271 / -22° .- 0.271/22° ; 0.182 H 

0.5 B 
o — VvV- 

►2 a 


J0.4mH i25ptF 

Fig. 9-10 See Drill Prob. 9-9. 


D 1 Application of the complex forcing function 3(V 120,r! V to a certain network 
produces the source current 5e*<i2&»-f-36.9 ) ^ jf tne curre nt arrow is directed out 
of the plus-marked source terminal: (a) What power is entering the network at 
t = 0? (b) What is the maximum instantaneous power entering the network? 

□ 2 A black box containing only passive elements possesses four terminals, labeled 
A, B, C, and D. If a voltage source v AB = 100e' (4 ' +30 ° 1 V is applied, the response, 
v CD = .lOe'te- 120 "' V, is obtained. Findvcaify^ = : (a) 50e> u,+30 "\ (b) 50e> Ut - 3O ° ) ; 
(c) 20 cos 4f; (d) 30 sin [it - 45°); (e) 100e )<7 '+ 30 ° ) V. 

D 3 A yellow box containing only passive elements possesses four terminals, labeled 
1, 2, 3, and 4. If a current source, i in , = 10 cos (lOOOf - 20°) A, is applied be- 

\ out3 = 2 sin (lOOOf + 50°) A, is 
j = : (a) 5 sin (1000* - 30°); 


tween terminals 1 and 2, then the response, t ( 
obtained at terminals 3 and 4. Find i„ 


(b) 6e' 10mt ; (c) j5e )(1000(+20 ° , ; (d) (8 + j6) e ' ( ioo»'+3o-) A . 

D 4 Given four nodes 1, 2, 
V 32 = -40 + /30, and V 34 

3, and 4, and the phasor voltages V 12 = 20 + ;50, 
= 30 /45° V, find t>,. at ut = 30°. 

D S Find v^t) and o 2 (t) if (2 
1000 rad/s. 

■ /!)% - /3V 2 = 10, -pV! + 4V 2 = -6, and u = 

D 6 If three currents entering a node are 10 cos (wf — 40°), 8 cos {ut — 100°), and 
15 sin {ut + 30°) A, find the current i 4 (t) leaving the node in the fourth conductor. 

□ 7 The phasor current, I = 10 — p A at u = 500 rad/s, is present in a certain 
circuit element. Find the power being delivered to the element at t = -ir ms if 
the element is: (a) a 2-S2 resistor; (b) a 4-mH inductor; (c) a 1000-pF capacitor; 
(d) a voltage source, V = 10 + ;20 V. 

□ 8 The voltage 20 cos (2000t + 60°) V is applied to a circuit element, and the 
current l m cos {oit + <t>) results, (a) Find <o, tf>, and L if the element is an inductor 
and I m = 0.1 A. (b) Find <o, <j>, and C if the element is a capacitor and l m = 0.1 A. 


267 The Phasor Concept 

D9 A 200-J2 resistor, a 0.04-H inductor, and a 0.25-juF capacitor are connected 
in series. Find the phasor voltage across the combination if the phasor current, 
30 /45° mA, is applied at co = : (a) 8000 rad/s; (b) 10,000 rad/s; (c) 12,500 rad/s. 

□ 10 A 0.5-ju.F capacitor, an 80-mH inductor, and a 500-fi resistor are in parallel 
with the voltage source, 12 — /6 V. Find the source current as a phasor if a = : 

(a) 500 rad/s; (b) 5000 rad/s; (c) 50,000 rad/s. 

□ 1 1 If the remaining two terminals are left open-circuited and w = 1 krad/s, find 
the input impedance of the network shown in Fig. 9-11 at terminals: (a) a-b; 

(b) c-d; (c) a-c. (d) Find Z jn at c-d if a and b are short-circuited. 

50 mi l 

_ impr*— 

10 /iF 

20 jiF 

Fi 9 . 9-11 See Prob. 11. 

□ 12 Find the impedance seen at terminals 1-2 in Fig. 9-12 at w = 0.1 Mrad/s 
if the network is cut at point: (d) x; (b) y; (c) z. (d) What is the impedance of 
the network as shown? 

Fig. 9-12 See Prob. 12. 

□ 1 3 A 60-fi resistor is in series with a 5-mH inductor. What size capacitor should 
be placed in parallel with this series combination so that the impedance of the 
parallel combination has zero reactance at <o = 24 krad/s? 

□ 1 4 A 20-fi resistor is in parallel with an inductor L; u = 10 3 rad/s. Find L so 
that: (a) resistive part of impedance of parallel combination is 8 U; (b) reactive 
part of impedance of parallel combination is 10 ft; (c) magnitude of impedance of 
parallel combination is 10 fi. 

□ 15 Let each inductor in the circuit shown in Fig. 9-13 be 2 H, and let each 
capacitor be % juF. Find Z in at a = 1000 rad/s if R = : (a) 0; (b) oo; (c) 1 kfi. 

Fig. 9-13 See Prob. 15. 

□ 16 Find Y jn for the network shown in Fig. 9-14 at u = 10* rad/s if G = : 

(c) 00; (b) 0. 


Fig. 9-14 See Prob. 16. 

D 17 A 5-kfl resistor and a capacitor C are in series. Let u = 10 7 rad/s. Find 
C so that: (a) the conductive part of the input admittance is 100 jjO; (b) the 
susceptive part of Y in is 50 fiU; (c) the angle of Y in is 60°. 

D 18 Between terminals a and fo is a capacitance C in series with the parallel 
combination of a 2000-fi resistor and a 2-mH coil. Find C so that the susceptive 
part of the input admittance is zero at 20 kHz. 

□ 19 If u = 10 4 rad/s, what two circuit elements connected in parallel would 
provide the same admittance as a 500-fi resistor and a 0.1-juF capacitor connected 
in series? 

□ 20 Find L and C so that the input impedance of the circuit shown in Fig. 9-15 
is 2R at u ~ <o . 

□ 21 The admittance and the impedance of the network shown in Fig. 9-16 are 
equal at every frequency. Find R and C. 

Fig. 9-16 See Prob. 21. 

Fig. 9-15 See Prob. 20. 


Z. = Y. 

JlH ^C 







The Sinusoidal 




In Chap. 2 and* particularly, Chap. 3 we learned a number of methods 
which are useful in analyzing resistive circuits. No matter what the com- 
plexity of the resistive circuit is, we are able to determine any desired 
response by asing nodal, mesh, or loop analysis, superposition, source. 
fcransformalfeiS, <& Thevenin's or Norton's theorems. Sometimes one 
Sietliodfe*ia^eM(,fa* more often we find it convenient to combine several 
i'- taetbodrlaot c Syma^vm -response in the most direct manner. We now wish 
to extend tfiese tecliabiques to the analysis of circuits in the sinusoidal steady 
state, and we lakve already seen that impedances combine in the same 

270 Sinusoidal Analysis 

manner as do resistances. The extension of the techniques of resistive circuit 
analysis has been promised several times, and we must now find out why 
the extension is justified and practice its use. 


Let us first review the arguments by which we accepted nodal analysis 
for a purely resistive circuit. After designating a reference node and 
assigning voltage variables between each of the N — 1 remaining nodes 
and the reference, we applied Kirchhoff's current law to each of these 
N — 1 nodes. The application of Ohm's law to all the resistors then led 
to N — 1 equations in N — 1 unknowns if no voltage sources or dependent 
sources were present; if they were, additional equations were written in 
accordance with the definitions of the types of sources involved. 

Now, is a similar procedure valid in terms of phasors and impedances 
for the sinusoidal steady state? We already know that both of Kirchhoff's 
laws are valid for phasors; also, we have an Ohm-like law for the passive 
elements, E = ZI. In other words, the laws upon which nodal analysis rests 
are true for phasors, and we may proceed, therefore, to analyze circuits 
by nodal techniques in the sinusoidal steady state. It is also evident that 
mesh- and loop-analysis methods are valid as well. 

As an example of nodal analysis, consider the frequency-domain circuit 
shown in Fig. 10-1. Each passive element is specified by its impedance, 
although the analysis might be simplified slightly by using admittance 
values. Two current sources are given as phasors, and phasor node voltages 
Vj and V 2 are indicated. At the left node we apply Kirchhoff's current 
law and I = E/Z, 

5 — /10 — p /10 

At the right node, 


^ + Y ^7~ + ^ + ^=-(-P- 

/10 ;5 10 


Fig. 10-1 A frequency-domain circuit for which node voltages V x and V 2 
are identified. 

~ -* 5n .> 

Ref. node 


i ion 

($) 0.5^/nM! 

27 1 The Sinusoidal Steady-state Response 

Combining terms, we have 

(0.2 + 10.2)% - j0.1V 2 = 1 (i) 

and -/O.lVj + (0.1 - /0.1)V 2 = /0.5 (2) 

Using determinants to solve (1) and (2), we obtain 

I 1 -jO-1 I 
v I ?0.5 (0.1 - /0.1) 1 Q.i - ft.i _ 0.Q5 

1 I (0.2 + /0.2) -/O.l I _ 0.02 - /0.02 + /0.02 + 0.02 + 0.01 
I -/0.1 (0.1-/0.1)1 

0.05 — »0.1 

= <—— = 1 - j2 V 

0.05 ' 

I (0.2 + p.2) 1 I 

v 2 J ~< - 1 g^ = -0-i + /0-i + /0-i = _ 2+4 v 

2 • 0.05 0.05 + ? 

The time-domain solutions are therefore obtained by expressing V, and 
V 2 in polar form, 

Vj = 2.24 / -63.4° V 2 = 4.47 /116.6° 

and passing to the time domain: 

v t (t) = 2.24 cos (at - 63.4°) v 2 (t) = 4.47 cos (at + 116.6°) V 

Note that the value of to would have to be known in order to compute 
the impedance values given on the circuit diagram. Also, both sources are 
assumed to operate at the same frequency. 

As an example of loop or mesh analysis, we consider the circuit given 
in Fig. 10-2a. Noting from the left source that <o = 10 3 rad/s, we draw 
the frequency-domain circuit of Fig. 10-26 and assign mesh currents I, 
and I 2 . Around mesh 1, 

3^ + m^ - h) = w/fli 

or (3 + j4)l t - /4I 2 = 10 

Fig. 10-2 (a) A time-domain circuit containing a dependent source, [b) The 
corresponding frequency-domain circuit on which mesh currents l x and I 2 
are indicated. 

272 Sinusoidal Analysis 

while mesh 2 leads to 


/4(I 2 - 1^-/212 + 2^=0 
(2 - /^ + /2I, = 


14 + /8 

= 1.24 /29.8° A 

l2= 20 + J30 =277Z5M1 A 

or i^t) = 1.24 cos (10 3 t + 29.8°) A 

i 2 (t) = 2.77 cos (10 3 f + 56.3°) A 

The solutions for either of the problems above could be checked by 
working entirely in the time domain, but it would be quite an undertaking 
and one which is typical of those we may safely ignore because the phasor 
method is providentially available. 

Drill Problems 

10-1 Use nodal analysis on the circuit shown in Fig. 10-3 to evaluate the phasor 
voltage: (a) V x ; (b) V 2 ; (c) V 3 . 

Ans. -105 - jl5; 15 - jlOS; 90 + J120 V 


>a> <! 

^>30fl I /30J2 


[$) =T=a ^6on 

Fig. 10-3 See Drill Prob. 10-1. 

10-2 In the circuit shown in Fig. 10-4, find: (a) 1 ± ; (b) I 2 ; (c) I 3 . 

Ans. -3 - j2; -1 + j2; 6 + JO A 

(a = 4 krad/s 

Fig. 10-4 See Drill Prob. lQr-2. 

10 Q 

273 Th * Sinusoidal Steady-state Respenu 


After inductance and capacitance were introduced in Chap. 4, we found 
that circuits containing these elements were still linear, and that the benefits 
of linearity were again available. Included among these were the super- 
position principle and Thevenin's and Norton's theorems; source trans- 
formations we now recognize as a simple case of the latter two theorems. 
Thus, we know that these methods may be used on the circuits we are 
now considering; the fact that we happen to be applying sinusoidal sources 
and are seeking only the forced response is immaterial. The fact that we 
are analyzing the circuits in terms of phasors is also immaterial; they are 
still linear circuits. We might also remember that linearity and superposi- 
tion were invoked when we combined real and imaginary sources to obtain 
a complex source. 

We therefore shall consider several examples in which answers are 
obtained more readily through applying superposition, source trans- 
formations, or Thevenin's or Norton's theorems. 

First we look again at the circuit of Fig. 10-1, redrawn as Fig. 10-5 
with each pair of parallel impedances replaced by a single equivalent 
impedance. That is, 5 and -;10 in parallel yield 4 - j2Q, ;10 in parallel 
with -/5 gives -;10 Q, and 10 in parallel with ;5 provides 2 + j4 fl. To 
find V lt we first activate only the left source and find the partial response 

V _ 1/0 . ( 4 -y2)(-/10 + 2 + /4) -4 
u 4-j2-jl0 + 2 + j4~ 6 - 


With only the right source active, current division helps us to obtain 

Vu, = (-0, 5/-9(n 


2 + /4 

j2 -jio + 2 + J4 

**)<«- «-^ — 

Fig. 10-5 \ 1 and V 2 may be found by using superposition of the separate 
phasor responses. 





($) «-5 tuse 


274 Sinusoidal Analysis 

Summing, then 

Vj = 2 - /2 - 1 = 1 - ;2 V 

which agrees with our previous result. 

We might also see whether or not Thevenin's theorem can help the 
analysis of this circuit (Fig. 10-5). Suppose we determine the Thevenin 
equivalent faced by the — /10-0 impedance; the open-circuit voltage ( + 
reference to left) is 

V oc = (1Z0!)(4 - /2) + (0.5 /-90°) (2 + /4) 
= 4-/2 + 2-/1 = 6-/3 

The impedance of the inactive circuit, as viewed from the load terminals, 
is simply the sum of the two remaining impedances. Hence, 

Z (ft = 6 + /2 

Thus, when we reconnect the circuit, the current directed from node 1 
toward node 2 through the — /'10-0 load is 

* - 6_/ ' 3 = 0.6 + f0.3 

6 + /2 - ;10 

Subtracting this from the left source current, the downward current through 
the 4 — /2-S2 branch is found: 

Ij = 1 - 0.6 - /0.3 = 0.4 - /0.3 
and, thus, 

V t = (0.4 - /0.3)(4 - /2) = 1-/2 V 

We might have been cleverer and used Norton's theorem on the three 
right elements, assuming that our chief interest is in V r Source trans- 
formations can also be used repeatedly to simplify the circuit. Thus, all 
the shortcuts and tricks that arose in Chaps. 2 and 3 are available for circuit 
analysis in the frequency domain. The slight additional complexity that 
is apparent now arises from the necessity of using complex numbers and 
not from any more involved theoretical considerations. 

Finally, we should also be pleased to hear that these same techniques 
will be applicable to the forced response of circuits driven by damped 
sinusoidal forcing functions, exponential forcing functions, and forcing 
functions having a complex frequency in general. Thus, we shall meet these 
same techniques again in Chap. 13. 

275 The Sinusoidal Steady-state Response 

Drill Problems 

10-3 Using superposition to find I in the circuit shown in Fig. 10-6, what is 
the partial (phasor) response produced by the: (a) left source? (b) right source? 
(c) upper source? 

Ans. 1.414; 1 - jl; 1 + jl A 

£ cos (I0*t - 4S°) A 

Fig. 10-6 See Drill Probs. 10-3 and 10-4. 

10-4 Assume that the 2-fi resistor is the load in Fig. 10-6 and determine the 
Thevenin equivalent of the circuit to which it is connected. Then calculate I 
if the load attached to the equivalent circuit is an impedance, Z L = : (a) 2 + f0 fi; 

(b) 2 - /2 U- (c) 2 + /2 U. 

Ans. 2.1 6/ -18.4° ; 3.41/0?; 4.83 /45° A 


The phasor diagram is a name given to a sketch in the complex plane of 
the phasor voltages and phasor currents throughout a specific circuit. It 
provides a graphical method for solving certain problems in which the 
complex algebraic calculations are tedious; it serves as a check on more 
exact analytical methods; and it proves to be of considerable help in 
simplifying the analytical work in certain symmetrical problems by enabling 
the symmetry to be recognized and helpfully applied. In the following 
chapter we shall encounter similar diagrams which display the complex 
power relationships in the sinusoidal steady state. The use of other complex 
planes will also appear in connection with complex frequency in Chap. 13. 
We are already familiar with the use of the complex plane in the 
graphical identification of a complex number and in their addition and 
subtraction. Since phasor voltages and currents are complex numbers, they 
may also be identified as points in a complex plane. For example, the phasor 
voltage \ = 6 + ;8 = 10 /53.1° is identified on the complex voltage plane 
shown in Fig. 10-7. The axes are the real voltage axis and the imaginary 

> Real axis (V) 

Fig. 10-7 A simple phasor diagram shows the single voltage phasor 
V, = 6 + ;8 = 10 /53.1° V. 

voltage axis; the voltage V t is located by an arrow drawn from the origin. 
Since addition and subtraction are particularly easy to perform and display 
on a complex plane, it is apparent that phasors may be easily added and 
subtracted in a phasor diagram. Multiplication and division result in the 
addition and subtraction of angles and a change of amplitude; the latter 
is less clearly shown, since the amplitude change depends on the amplitude 
of each phasor and on the scale of the diagram. Figure 10-8a shows the 
sum of V a and a second phasor voltage V 2 = 3 - /4 = 5 /-53.1" and Fig. 
10-8fo shows the current I 1? which is the product of V x and the admittance 

Y = 1 + /'l. 

This last phasor diagram shows both current and voltage phasors on 
the same complex plane; it is understood that each will have its own 
amplitude scale, but a common angle scale. For example, a phasor voltage 
1 cm long might represent 100 V, while a phasor current 1 cm long could 
indicate 3 mA. 

Fig. 10-8 (a) A phasor diagram showing the sum of Vj = 6 + /8 and 
V 2 = 3 - ;4, Vj + V 2 = V + /4 = 9.85 /24.0° . (fc) The phasor diagram 
shows Vj and I 1; where Ij = Y^ and Y = 1 + jl G. 

v, +v. 


/ut + a 



Fig. 10-9 (a) The phasor voltage V„/a. (fc) The complex voltooe V n /ut + a 
is shown as a phasor at a particular instant of time. This phasor leads V„Za 
by ut rod. 

The phasor diagram also offers an interesting interpretation of the 
time-domain to frequency-domain transformation, since the diagram may 
be interpreted from either the time- or frequency-domain viewpoint. Up 
to this time, it is obvious that we have been using the frequency-domain 
interpretation, because we have been showing phasors directly on the 
phasor diagram. However, let us proceed to a time-domain viewpoint by 
first showing the phasor V = V m /a, as sketched in Fig. 10-9a. In order 
to transform V to the time domain, the next necessary step is the multi- 
plication of the phasor by e iut ; thus we have the complex voltage V m e ia e iat = 
V m /ut + a . This voltage may also be interpreted as a phasor, one which 
possesses a phase angle which increases linearly with time. On a phasor 
diagram it therefore represents a rotating line segment, the instantaneous 
position being cor rad ahead (counterclockwise) of V m /a_ . Both V m /a. and 
V^ /cor + a are shown on the phasor diagram of Fig. 10-9fo. 

The passage to the time domain is now completed by taking the real 
part of V m /tor + a. The real part of this complex quantity, however, is 
merely the projection of VL /W + a on the real axis. In summary, then, 
the frequency-domain phasor appears on the phasor diagram, and the 
transformation to the time domain is accomplished by allowing the phasor 
to rotate in a counterclockwise direction at an angular velocity of co rad/s 
and then visualizing the projection on the real axis. It is helpful to think of 
the arrow representing the phasor V on the phasor diagram as the snapshot, 
taken at uit = 0, of a rotating arrow whose projection on the real axis is the 
instantaneous voltage v(i). 

Let us now construct the phasor. diagrams for several simple circuits. 
The series RLC circuit shown in Fig. 10- 10a has several different voltages 
associated with it, but only a single current. The phasor diagram is con- 
structed most easily by employing the single current as the reference 
phasor. Let us arbitrarily select I = Z m /0° and place it along the real axis 
of the phasor diagram, Fig. 10- 10b. The resistor, capacitor, and inductor 

JU. ; 50Q 10 n 

-mtf* VW 

+ \~ + v B 


-iso a 


Fig. 10-10 (a) A series RLC circuit shown in the frequency domain. 
[b] The associated phasor diagram, drawn with the single mesh current as the 
reference phasor. 

voltages may next be calculated and placed on the diagram, where the 
90° phase relationships stand out clearly. The sum of these three voltages 
is the source voltage, and for this circuit, which is in the resonant condition 1 
where Z c = -Z L , the source voltage and resistor voltage are equal. The 
total voltage across the resistance and inductance or resistance and capaci- 
tance is easily obtained from the phasor diagram. 

The phasor diagram may be interpreted in the time domain by allowing 
all the phasors to rotate synchronously with a counterclockwise angular 
velocity of to rad/s, and then considering the projections on the real axis. 

Figure 10-lla shows a simple parallel circuit in which it is logical to 
use the single voltage between the two nodes as a reference phasor. Suppose 
that V = 1/01 V. The resistor current is in phase with this voltage, 1 R = 
0.2/0° A, and the capacitor current leads the reference voltage by 90°, 
l c = /0.1 A. After these two currents are added to the phasor diagram, 
shown as Fig. 10-1 lb, they may be summed to obtain the source current. 
The result is I s = 0.2 + /0.1 A. 

If the source current were specified initially as, for example, 1/01 A, 
and the node voltage is not initially known, it is still convenient to begin 
construction of the phasor diagram by assuming a node voltage, say V = 
1 /0" V once again, and using it as the reference phasor. The diagram is 
then completed as before, and the source current which flows as a result 
of the assumed node voltage is again found to be 0.2 + /0.1 A. The true 
source current is 1/01 A, however, and thus the true node voltage is greater 
by the factor 1/01/(0.2 + /0.1); the true node voltage is therefore 4 - ft V. 

•Resonance will be denned in Chap. 14. 



2000 rad/j 




5$i< V 50/zF-fc 

I, = 0.2 + (O.I 



Rg. 10-1 ? (a) A parallel RC circuit, (fe) The phasor diagram for this cir- 
cuit; the node voltage V is used as a convenient reference phasor. 

The assumed voltage leads to a phasor diagram which differs from the true 
phasor diagram by a change of scale (the assumed diagram is smaller by 
a factor of 1/ \/20) and an angular rotation (the assumed diagram is rotated 
counterclockwise through 26.6°). 

Phasor diagrams are usually very simple to construct, and most sinus- 
oidal steady-state analyses will be more meaningful if such a diagram is 
included. Additional examples of the use of phasor diagrams will appear 
frequently throughout the remainder of our study. 

Drill Problems 

10-5 Analyze the circuit shown in Fig. 10- 12a by constructing a reasonably 
accurate phasor diagram with the voltage Vj as the reference phasor. Let the 
arrow representing Vj be 2 in. long at an angle of 0°, and let the I x arrow be 3 in. 
long. What is the length of the arrow for: (a) I 3 ; (b) 1^ (c) V s ? 

Ans. 1.50; 2.24; 3.35 in. 

10-6 A phasor diagram is constructed for the circuit shown in Fig. 10- 12b. The 
scale used is 20 V/in. and 0.4 A/in. If Vj is represented by an arrow 1.6 in. long 
at an angle of —90°, V 2 by a 2-in. long arrow at an angle <f>, and I s by a 1.8-in. 
long arrow at an angle of —90°, find the impedance of the: (a) capacitor; (b) 
resistor; (c) inductor. 

Ans. 25; —J33.3; J33.3 Q 
R9. 10-12 (a) See Drill Prob. 10-5. [b) See Drill Prob. 10-6. 

100 is. 
v. = v 

jio n 


-j2o n 



280 Sinusoidal Analysis 


We will now consider methods of obtaining and presenting the response 
of a circuit with sinusoidal excitation as a function of the radian frequency 
co. With the possible exception of the 60-Hz power area in which frequency 
is a constant and the load is the variable, sinusoidal frequency response 
will be seen to be extremely important in almost every branch of electrical 
engineering as well as in related areas, such as the theory of mechanical 

Let us suppose that we have a circuit which is excited by a single source 
V, = V,/0- This phasor voltage may also be transformed into the time- 
domain source voltage V 8 cos (ut + 6). Somewhere in the circuit exists the 
desired response, the current I. As we know, this phasor response is a 
complex number, and its value cannot be specified in general without the 
use of two quantities: either a real part and an imaginary part, or a 
magnitude and a phase angle. The latter pair of quantities is more useful 
and more easily determined experimentally, and it is the information which 
we shall obtain analytically as a function of frequency. The data may be 
presented as two curves, the magnitude of the response as a function of 
co and the phase angle of the response as a function of u. We often 
normalize the curves by plotting the magnitude of the current-voltage ratio 
and the phase angle of the current-voltage ratio versus co. It is evident 
that an alternative description of the resultant curves is the magnitude and 
phase angle of an admittance as a function of frequency. A normalized 
voltage response may be similarly presented as the magnitude and phase 
angle of an impedance versus co. Other possibilities are voltage-voltage 
ratios (voltage gains) or current-current ratios (current gains). Let us 
consider the details of this process by thoroughly discussing several exam- 

For the first example, let us select the series RL circuit. The phasor 
voltage V, is therefore applied to this simple circuit, and the phasor current 
I is selected as the desired response. We are dealing with the forced 
response only, and the familiar phasor methods enable the current to be 


1 = 

R + juL 

Let us immediately express this result in normalized form as a ratio of 
current to voltage, that is, as an input admittance: 

or Y = „ *, T (3) 

R + juL w 

281 The Sinusoidal Steady-state Response 

If we like, we may consider the admittance as the current produced by 
a source voltage 1/01 V. The magnitude of the response is 

IYI = 1 (4) 

while the angle of the response is found to be 

ang Y = -tan- 1 -^ (5) 

Equations (4) and (5) are the analytical expressions for the magnitude and 
phase angle of the response as a function of to; we now desire to present 
this same information graphically. 

We shall first consider the magnitude curve. The first important factor 
to note is that we are plotting the absolute magnitude of some quantity 
versus <o, and the entire curve must therefore lie abotie the to axis. The 
response curve is constructed by noting that the value of the response at 
zero frequency is 1/R, that the initial slope is zero, and that the response 
approaches zero as frequency approaches infinity; the graph of the magni- 
tude of the response as a function of to is shown in Fig. 10-13a. 

For the sake of generality and completeness, the response is shown for 
both positive and negative values of frequency; the symmetry results from 
the fact that (4) indicates that |Y| has the same value when to is replaced 
by (—to). The physical interpretation of a negative radian frequency, such 
as oi = —100 rad/s, depends on the time-domain function, and it may 
always be obtained by inspection of the time-domain expression. Suppose, 
for example, that we consider the voltage v(t) = 50 cos (cot + 30°). At 
<o = 100, the voltage is v(t) = 50 cos(100t + 30°), while at to = -100, 
u(t) = 50 cos (-100t + 30°) or 50 cos (lOOt - 30°). Any sinusoidal re- 
sponse may be treated in a similar manner. 

The second part of the response, the phase angle of Y versus o>, is an 
inverse tangent function. The tangent function itself is quite familiar, and 
we should have no difficulty in turning that curve on its side; asymptotes 
of plus and minus 90° are helpful. The response curve is shown in Fig. 
10-136. The points at which to = ±R/L are marked on both the magnitude 
and phase curves. At these frequencies the magnitude is 0.707 of the 
maximum magnitude at zero frequency and the phase angle has a magnitude 
of 45° . At the frequency at which the admittance magnitude is 0.707 times 
its maximum value, the current magnitude is 0.707 times its maximum 
value, and the average power supplied by the source is 0.707 2 or 0.5 times 
its maximum value. It is not very strange that to = R/L is identified as 
a half-power frequency. 

As a second example, let us select a parallel LC circuit driven by a 


Fig. 10-13 (a) The magnitude of Y = I/V, and [b) the angle of Y are 
plotted as functions of w for a series KL circuit with sinusoidal excitation. 

sinusoidal current source, as illustrated in Fig. 10- 14a. The voltage response 
V is easily obtained: 

V = I. 


s /coL - /(1/<oC) 
and it may be expressed as an input impedance 


Z = ^ = 

I, faL - 1/uC) 

Z = i 1 <•> 

' C u 2 - 1/LC 


By letting 



ang Z 

-> « 


Hg. 10-14 (a) A sinusoidally excited parallel LC circuit, {b) The magni- 
tude of the input impedance, Z = V/I fl , and (c) the angle of the input 
impedance are plotted as functions of w. 

and factoring the expression for the input impedance, 

|Z| = 


C |(io - w )(w + w )| 


the magnitude of the impedance may be written in a form which enables 
those frequencies to be identified at which the response is zero or infinite. 
Such frequencies are termed critical frequencies, and their early identifica- 
tion simplifies the construction of the response curve showing amplitude 
versus frequency. We note first that a zero-amplitude response occurs at 
co = 0; such a response as well as the frequency at which it occurs is called 
a zero. Response of infinite amplitude is noted at co = co and co = — co ; 
these frequencies are called poles, as is the infinite-amplitude response 
itself. Finally, we note that the response approaches zero as co — » oo, and 
thus co = ±oo is also a zero. 2 

The locations of the critical frequencies should be marked on the co 

2 It is customary to consider plus infinity and minus infinity as being the same point. The phase 
angle of the response at very large positive and negative values of w need not be the same, 


284 Sinusoidal Analysis 

axis, by using small circles for the zeros and crosses for the poles. Poles 
or zeros at infinite frequency should be indicated by an arrow near the 
axis, as shown in Fig. 10-14&. The actual drawing of the graph is made 
easier by adding broken vertical lines as asymptotes at each pole location. 
The completed graph of magnitude versus <o is shown in Fig. 10- 14b; the 
slope at the origin is not zero. 

An inspection of (6) shows that the phase angle of the input impedance 
must be either +90 or —90°; no other values are possible, as must appar- 
ently be the case for any circuit composed entirely of inductors and 
capacitors. An analytical expression for ang Z would therefore consist of 
a series of statements that the angle is +90 or —90° in certain frequency 
ranges. It is simpler to present the information graphically, as shown in 
Fig. 10- 14c. Although this curve is only a collection of horizontal straight 
line segments, errors are often made in its construction, and it is a good 
idea to make certain that it can be drawn directly from an inspection of 

Drill Problems 

10-7 A 4-kfl resistor, a 10-ftF capacitor, and a sinusoidal current source l a are 
in parallel. Sketch as a function of «: (a) the magnitude of the voltage across 
the source; (b) the magnitude of the ratio of the voltage across the source to the 
source current; (c) the phase angle of the ratio of the voltage across the source 
to the source current. As a check on the results, the answers given below apply 
to o> = 25 rad/s. 

Ans. 2.83 fcfi; 2830 |I,| V; -45° 

10-8 A 3-/iF capacitor, a sinusoidal source V s , and the parallel combination of 
1 jiF and % H are all in series. Let the desired response be the ratio of the 3-/uF 
capacitor voltage to the source voltage. Sketch the magnitude and phase angle 
of the response as a function of gj and determine all critical frequencies of the 

Ans. ±1000; ±2000 rad/s 


□ 1 (a) Find V 2 in the circuit shown in Fig. 10-15. (b) What is v 2 (t) if w = 500 rad/s? 
(c) Find V 2 if the 2-fi resistor is replaced by a dependent current source, 0.5V 2 , 
reference arrow directed upward. 

D 2 For the ladder network shown in Fig. 10-16, find V oui if V in = 100/0° mV 
at (0 = 100 rad/s. 

2 a 

Fig. 10-15 See Prob. 1. 

0.5 juF 0.5 juF 0.5 juF 0.5 jjF 

o K 1 K T K T K— 

v in 10 va< 


10 kn< 

iokn?v ou , 

Fig. 10-16 See Prob. 2. 
□ 3 Find vjt) in the circuit shown in Fig. 10-17. 

Fig. 10-17 See Prob. 3. 
D 4 If u = 2 X 10 5 rad/s, find vj,t) for the circuit of Fig. 10-18. 
Fig. 10-18 See Probs. 4 and 7. 


286 Sinusoidal Analysis 

□ 5 Find i for the circuit shown in Fig. 10-19. 

10 cos IO 6 t f + 

Fig. 10-19 See Prob. 5. 

+/| 10 cos 2 X 10 s t 

□ 6 Find the ratio of |I 2 | to |I S | in the circuit shown in Fig. 10-20 if w = : (a) 
200; (b) 2000; (c) 20,000 rad/s. 

Fig. 10-20 See Prob. 6. 

D 7 Find the Thevenin equivalent of that portion of the circuit of Fig. 10-18 that 
is to the right of the current source. Let <o = 10 5 rad/s. 

D 8 A linear network containing one or more sinusoidal sources operating at 
2 krad/s has two accessible terminals, a and b. When a 50-fi resistor, a 2.5-jitF 
capacitor, and a 50-mH inductor are independently placed between the terminals, 
the magnitude of V ab is found to be 25, 100, and 50 V, respectively. Determine 
the Thevenin equivalent of the unknown network. 

□ 9 With reference to terminals a-b and load Z L in the circuit shown in Fig. 10-21, 
find the open-circuit voltage, the short circuit current, and draw the Norton 
equivalent circuit. What value of Z t will result in the greatest magnitude of load 

2/2° A (J) 



'io a 

Fig. 10-21 See Prob. 9. 

D 10 Find i t and t> 2 in the circuit shown in Fig. 10-22. 

D 1 1 (a) What is the maximum voltage present across the capacitor and resistor 

8 A 

Fig. 10-22 See Prob. 10. 

in the circuit of Fig. 10-23? (b) Replace the current source and capacitor by an 
equivalent series combination of a voltage source and a capacitor. Again deter- 
mine the two maximum voltages. 

10 kn 

Fig. 10-23 See Prob. 11. 

□ 12 In the circuit shown in Fig. 10-24, the values of R v R 2 , and V„ are unknown. 
Determine the value of C so that i x = at u = <o r 

Fig. 10-24 See Prob. 12. 

□ 1 3 A voltage 100 cos 500* V is applied to Zj and Z 2 in series. The amplitudes 
of the voltages across Z a and Z 2 are found to be 100 V and 125 V, respectively. 
If it is known that Z 2 is composed of R ± and Lj in series, where R 1 = 1 Q: (a) 
construct a phasor diagram and use it to determine L t ; (b) find Lj without using 
a phasor diagram. 

□ 14 A parallel RLC circuit with R = 200 Q, L = 10 mH, and C = 1 pF is excited 
by a parallel current source, I s = 2 /0° mA. Show the element currents and 
voltages on a phasor diagram for: (a) to = 10 4 ; (b) a = 5000 rad/s. 


288 Sinuioidol Analytic 

□ 15 Sketch curves of the magnitude and phase angle of V x as functions of to for 
the circuit of Fig. 10-25. Identify the half-power frequency. 

V_ cos oil ( ~ 

Fig. 10-25 See Probs. 15 and 16. 

□ 16 (a) Sketch curves of the magnitude and phase angle of V 2 as functions of 
w for the circuit of Fig. 10-25. (b) What is the greatest difference in phase angle 
between V 2 and the source voltage? 

□ 17 A certain physical coil is modeled by the series combination of a 200-J2 
resistance and a 50-mH inductance. The coil is placed in series with a 0.2-jitF 
capacitance and a voltage source, 10 cos ut mV. What is the maximum voltage 
that appears across the: (a) inductor; (b) coil? 

□ 1 8 For the network shown in Fig. 10-26, sketch |Z jn | and ang Z in versus o> if the 
4-/iF capacitor is: (a) short-circuited; (b) left as is. 

1 mH 

4 fie 

Fig. 10-26 See Prob. 18. 

□ 19 Sketch a curve showing the magnitude of the voltage across the source as 
a function of w for < « < 5 for the circuit shown in Fig. 10-27. 

□ 20 Sketch a curve of |Y jn | versus <o for the network shown in Fig. 10-28 if k = : 
(a) 0; (b) 100. 

Fig. 10-27 See Prob. 19. 





'i a 

=fei F 

Fig. 10-28 See Prob. 20. 


I 1 " 
100 fi =t= 1 *" F 

lti MBri - 




— i 






MB , ^WI|ilMff@|l |l ''ii | »'- ri "M" Wi|iiifci'iiii<ii niiniijii iWffiBSjqmS 

p|p;Sfee3:*iiiite^ .is deA^i|||^^| 

i-%W.t^^te^^w^^ ,: «eqKM«e»i«*^ <teten8fc*(NL Primarily, ho^e^^S 
\\ We a*e concerned^^S' Ae rate at whicb e«^gj>' iS being generatttf-aHfl:'?^^ 
:£' absorbed; our at%^&«iustiio* be directed to potior. '>.!'-"?i 

290 Sinusoidal Analysis 

We shall begin by considering instantaneous power, the product of the 
time-domain voltage and time-domain current associated with the element 
in which we are interested. The instantaneous power is sometimes quite 
useful in its own right, because its maximum value might have to be limited 
in order to avoid exceeding the safe or useful operating range of a physical 
device. For example, transistor and vacuum-tube power amplifiers both 
produce a distorted output when the peak power exceeds a certain limiting 
value. However, we are mainly interested in instantaneous power for the 
simple reason that it provides us with the means to calculate a more 
important quantity, the average power. In a similar way, the progress of 
a cross-country automobile trip is best described by the average velocity; 
our interest in the instantaneous velocity is limited to the avoidance of 
maximum velocities which will endanger our safety or arouse the highway 

In practical problems we shall deal with values of average power which 
range from the small fraction of a picowatt available in a telemetry signal 
from outer space, the few watts of audio power supplied to the speakers 
in a high-fidelity stereo system, the several hundred watts required to in- 
vigorate the morning coffeepot, to the millions of watts needed to supply all 
the electrical needs of a large city. 

Our discussion will not be concerned entirely with the average power 
delivered by a sinusoidal current or voltage; we shall establish a mathe- 
matical measure of the effectiveness of other waveforms in delivering 
power, which we shall call the effective value. Our study of power will 
be completed by considering the descriptive quantities, power factor and 
complex power, two concepts which introduce the practical and economic 
aspects associated with the distribution of electric power. 


The power delivered to any device as a function of time is given by the 
product of the instantaneous voltage across the device and the instantaneous 
current through it, as we well know; the passive sign convention is assumed. 

p = vi (1) 

A knowledge of both the current and the voltage is presumed. If the device 
in question is a resistor R, then the power may be expressed solely in terms 
of either the current or the voltage, 

p = vi = « 2 fi = £- (2) 

29 1 Average Power and RMS Values 

If the voltage and current are associated with a device which is entirely 
inductive, then 

r di 1 r' J 
p = VI = i-'-T" = T v I ° <" (3) 

where we have arbitrarily assumed that the voltage is zero at t — — oo. 
In the case of a capacitor, 

dv 1 r' 
p = vi = Cv— = -i)jdt (4) 

where a like assumption about the current is made. This listing of equations 
for power in terms of only a current or voltage soon becomes unwieldy, 
however, as we begin to consider more general networks. The listing is 
also quite unnecessary, for we need only find both the current and voltage 
at the network terminals. As an example, we may consider the series RL 
circuit, as shown in Fig. 11-1, excited by a step- voltage source. The familiar 
current response is 

Kt) = §(1 - <r*' /L Mt) 

and thus the total power delivered by the source or absorbed by the passive 
network is 

p = vi = -^-(1 - e- Rt/L )u(t) 

since the square of the unit-step function is obviously the unit-step function 

The power delivered to the resistor is 

P* = * 2 « = -^(1 - e- B '^fu(t) 

Fig. 11-1 The power that is delivered to R is p B = i 2 R ■ 

(V 2 /fl)(l - e- R,/L ) 2 u[t)- 

v «(o( 

292 Sinusoidal Analysis 

In order to determine the power absorbed by the inductor, we first obtain 
the inductor voltage 

VL ~ L dt 

= v-*«y*) + ^(i - *-»"<)*§- 

since du(t)/dt is zero for t > and (1 - e - m/L ) is zero at t - 0. The 
power absorbed by the inductor is thus 

Pl = « L < = ^e-«'"(l - e-*»' L Mt) 

Only a few algebraic manipulations are required to show that 

P = Pr + Pl 

which serves to check our wprk. 

The majority of the problems which involve power calculations are 
perhaps those which deal with circuits excited by sinusoidal forcing func- 
tions in the steady state; as we have been told previously, even when 
periodic forcing functions which are not sinusoidal are employed, it is 
possible to resolve the problem into a number of subproblems in which 
the forcing functions are sinusoidal. The special case of the sinusoid 
therefore deserves special attention. 

Let us change the voltage source in the circuit of Fig. 11-1 to the 
sinusoidal source V m cos cot. The familiar time-domain response is 

i(t) = I m cos (at + 0) 


V aL 

I = . " and 6 = -tan- 1 

m Vfl 2 + a 2 L 2 R 

The instantaneous power delivered to the entire circuit in the sinusoidal 
steady state is, therefore, 

p = vi = V m I m cos (at + 8) cos at 

which we shall find convenient to rewrite in a form obtained by using the 
trigonometric identity for the product of two cosine functions. Thus, 

293 Average Power and RMS Values 

V / 

p = -2p4cos (2at + 6) + cos 8] 

Yolo. cos + ^22. cos (2(0t + 0) 

The last equation possesses several characteristics which are true in general 
for circuits in the sinusoidal steady state. One term, the first, is not a 
function of time; and a second term is included which has a cyclic variation 
at twice the applied frequency. Since this term is a cosine wave, and since 
sine waves and cosine waves have average values which are zero (when 
averaged over an integral number of periods), this introductory example 
may serve to indicate that the average power is Y 2 V m I m cos 0. This is true, 
and we shall now establish this relationship in more general terms. 

Drill Problems 

11-1 A current source, 8 cos500r A, a 5-fi resistor, and a 20-mH inductor are 
in parallel. At t = I ms find the power absorbed by the: (a) resistor; (b) inductor; 
(c) source. 

Am. -143; 60; 83 W 

11-2 A current source, 8u(t) A, a 5-S2 resistor, and a 20-mH inductor are in 
parallel. At t = 3 ms, find the power absorbed by the: (a) resistor; (b) inductor; 
(c) source. 

Am. -151; 71; 80 W 


When we speak of an average value for the instantaneous power, the time 
interval over which the averaging process takes place must be clearly 
defined. Let us first select a general interval of time from t 1 to t 2 . We 
may then obtain the average value by integrating p(t) from t x to t 2 and 
dividing the result by the time interval t 2 — t v Thus, 

1 c' 2 

*0 *1*'*- 



The average value is denoted by the capital letter P since it is not a function 
of time, and it usually appears without subscripts. Although P is not a 
function of time, it is a function of t ± and ( 2 , the two instants of time which 
define the interval of integration. This dependence of P on a specific time 

294 Sinusoidal Analysis 

interval may be expressed in a simpler manner if p(t) is a periodic function. 
We shall consider this important case first. 

Let us assume that our forcing function and the circuit responses are 
all periodic; a steady-state condition has been reached, although not neces- 
sarily the sinusoidal steady state. We may define a periodic function math- 
ematically by requiring that 

f(t) = f(t + T) (6) 

where T is the period. We now show that the average value of the instan- 
taneous power as expressed by (5) may be computed over an interval of one 
period having an arbitrary beginning. 

A general periodic waveform is shown in Fig. 11-2 and identified as 
p(t). We first compute the average power by integrating from t 1 to a time 
t 2 which is one period later, t 2 = t t + T, 

1 r H+T 
1 J ti 

and then by integrating from some other time t x to t x + T, 



p(t) dt 

The equality of P x and P x should be evident from the graphical inter- 
pretation of the integrals; the area which represents the integral to be 
evaluated in determining P x is smaller by the area from t t to t x , but greater 
by the area from t x + T to t x + T, and the periodic nature of the curve 
requires these two areas to be equal. Thus, the average power may be 
computed by integrating the instantaneous power over any interval which 
is one period in length and then dividing by the period 

1 r tlVT 
P = jj pdt (7) 


It is important to note that we might also integrate over any integral number 
of periods, provided that we divide by this same integral number of periods. 

P = -^.J pdt n = 1,2,3, ... (8) 

If we carry this concept to the extreme by integrating over all time, another 

F19. 11-2 The average value P of a periodic power function p(t) is the 
same over any period T. 

useful result is obtained. We first provide ourselves with symmetrical limits 
on the integral 

1 -IWV2 

P =^f! pdt 

and then take the limit as n becomes infinite, 

1 ~nin 
P = lim — I p 


If p(t) is a mathematically well-behaved function, as all physical forcing 
functions and responses are, it is apparent that if a large integer n is 
replaced by a slightly larger number which is not an integer, then the value 
of the integral and of P is changed by a negligible amount; moreover, the 
error decreases as n increases. Without justifying this step rigorously, we 
therefore replace the discrete variable nT by the continuous variable t, 

1 r rn 
P = lim - I pdt 

T _>oo T J_./o 


We shall find it convenient on several occasions to integrate periodic 
functions over this "infinite period." Examples of the use of (7), (8), and 
(9) are given below. 

Let us illustrate the calculation of the average power of a periodic wave 
by finding the average power delivered by the (periodic) sawtooth current 
waveform shown in Fig. 11 -3a to a resistor R. We have 

i(t) =-a< 0<t<T 

i(t) = J2.(t - T) T<t<2T 




Fig. 11 -3 [a] A sawtooth current waveform and (b) the instantaneous power 
waveform it produces in a resistor R. 


PM = ft V«' 2 o < t < T 

Pit) = filJW - Tf T<t< 



as sketched in Fig. 1 l-3fo. Integrating over the simplest range of one period, 
from t — to t = T, we have 

1 r T I 2 R 
P =tI h ^ Lt2 dt=y 3 I n ?R 

The selection of other ranges of one period, such as from t = 0.1T to 
t = LIT, would produce the same answer. Integration from to 2T and 
division by 2T, that is, the application of (8) with n = 2 and t x = 0, would 
also provide the same answer. 

Now let us obtain the general result for the sinusoidal steady state. 
We shall assume the general sinusoidal voltage 

v(t) = V m cos (ut + a) 
and current 

i(t) = I m cos (at + a - 6) 

associated with the device in question. The instantaneous power is 

p(t) = V m I m cos (at + a) cos (at + a — 6) 

Again expressing the product of two cosine functions as one-half the sum 

297 Avara 9* Power and RMS Valum 

of the cosine of the difference angle and the cosine of the sum angle, 

p(*) = % VJ. cos + V 2 V m I m cos (&»f + 2a - 9) (10) 

we may save ourselves some integration by an inspection of the result. 
The first term is a constant, independent of t. The remaining term is a 
cosine function; p(t) is therefore periodic, and its period is %T. Note that 
the period T is associated with the given current and voltage, and not with 
the power; the power function has a period ^/ 2 T. However, we may inte- 
grate over an interval of T to determine the average value if we wish; 
it is only necessary to divide also by T. Our familiarity with cosine and 
sine waves, however, shows that the average value of either over a period 
is zero. There is thus no need to integrate (10) formally; by inspection, 
the average value of the second term is zero over a period T (or %T), and 
the average value of the first term, a constant, must be that constant itself. 

P = 1 / 2 V m 4 l cos0 (11) 

This important result, introduced in the previous section for a specific 
circuit, is therefore quite general for the sinusoidal steady state. The 
average power is one-half the product of the crest amplitude of the voltage, 
the crest amplitude of the current, and the cosine of the phase-angle 
difference between the current and the voltage; the sense of the difference 
is immaterial. 

As a numerical illustration, let us assume that a voltage 

v{t) = 4cos^- 

or V = 4201 

is applied across an impedance Z = 2 /60° Si. The phasor current is 
therefore 2 /—60° A, and the average power is 

P = l / 2 (4)(2) cos 60° = 2 W 

The time-domain voltage 

»(f) = 4 cos 21 

time-domain current 

i(t) = 2 cos fa- - 60°) 

p, c, i » (W, V, A) 


Fig. 11-4 Curves of v[t), i(t), and p[t) are plotted as a function of time for a 
simple circuit in which the phasor voltage V = 4ZQ1 V is applied to the 
impedance Z = 2 /60° 8 al B = ir/6. 

and instantaneous power 

p(t) = 8cos^cos(^-60°) 
= 2 + 4cos(^-60°) 

are all sketched on the same time axis in Fig. 11-4. Both the 2-W average 
value of the power and its period of 6 s, one-half the period of either the 
current or the voltage, are evident. The zero value of the instantaneous 
power at each instant when either the voltage or current is zero is also 

Two special cases are worth isolating for consideration, the average 
power delivered to an ideal resistor and that to an ideal reactor (any 
combination of only capacitors and inductors). The phase-angle difference 
between the current through and the voltage across a pure resistor is zero, 
and therefore 


V 2 


The last two formulas, enabling us to determine the average power de- 
livered to a pure resistance from a knowledge of either the sinusoidal 
current or voltage, are simple and important. They are often misused. 
The most common error is made in trying to apply them in cases where, 
say, the voltage included in (13) is not the voltage across the resistor. If 
care is taken to use the current through the resistor in (12) and the voltage 
across the resistor in (13), satisfactory operation is guaranteed. 

The average power delivered to any device which is purely reactive 


Fig. 11-5 The average power delivered to each reactive element is zero in 
the sinusoidal steady state. 

must be zero. This is evident from the 90° phase difference which must 
exist between current and voltage; hence, cos — and 

P„ = 

The average power delivered to any network composed entirely of ideal 
inductors and capacitors is zero; the instantaneous power is zero only at 
specific instants. Thus, power flows into the network for a part of the cycle 
and out of the network during another portion of the cycle. 

As an example illustrating these relationships, let us consider the circuit 
shown in Fig. 11-5. The values of l t and I 2 are found by any of several 
methods, such as mesh analysis, nodal analysis, or superposition: 

Ii = 5 - ;10 = 11.1 8/-63.45 
I 2 = 5 - ;5 = 7.0 7/ -45° 

The current through the 2-U resistor is 

Ij - I 2 = -;5 = 5 /-90° 
and the resistor voltage is, therefore, 

V a = 10 /-90° 

This current and voltage satisfy the passive sign convention, and the average 
power absorbed by the resistor is, therefore, 

P R = y 2 (10)(5) cos (-90° + 90°) = 25 W 

a result which may be checked by using (12) or (13). Turning to the left 
source, the voltage 20 /0° and current 11.18 / — 63.45° satisfy the active 
sign convention, and thus the power delivered by this source is 


300 Sinusoidal Analysis 

In a similar manner, we find the power absorbed by the right source, 

? rish t = y 2 (10)(7.07) cos (0° + 45") = 25 W 

The power delivered to each of the two reactive elements is zero; the power 
relations check. 

In Sec. 4 of Chap. 3 we considered the maximum-power-transfer 
theorem as it applies to resistive loads and resistive source impedances. 
For a Thevenin source V 8 and impedance X th = R th + jX th connected to 
a load Z L = R L + jX L , it may he shown readily (Prob. 6) that the average 
power delivered to the load is a maximum when R L = R th and X h = — X th . 
This result is often dignified by calling it the maximum-power-transfer 
theorem for the sinusoidal steady state. It is apparent that the resistive 
condition considered earlier is merely a special case. 

We must now pay some attention to nonperiodic functions. One practi- 
cal example of a nonperiodic power function for which an average power 
value is desired is the power output of a radio telescope which is directed 
toward a "radio star." Another is the sum of a number of periodic functions, 
each function having a different period, such that no greater common 
period can be found for the combination. For example, the current 

i(t) = sin * + sin -at (14) 

is nonperiodic because the ratio of the periods of the two sine waves is 
an irrational number. At t = 0, both terms are zero and increasing. But 
the first term is zero and increasing only when t — 2-rm, where n is an 
integer, and thus periodicity demands that irt or -ni^nn) must equal 2mm, 
where m is also an integer. No solution (integral values for both m and 
n) for this equation is possible. It may be illuminating to compare the 
nonperiodic expression (14) with the periodic function 

i(t) = sin t + sin 3.14f (15) 

where 3.14 is an exact decimal expression and is not intended to be inter- 
preted as 3.141592 .... With a little effort, it can be shown that the 
period of this current wave is lOOw s. 

The average value of the power delivered to a 1-0 resistor by either 
the periodic current (15) or the nonperiodic current (14) may be found 
by integrating over an infinite interval; much of the actual integration can 
be avoided because of our thorough knowledge of the average value of 
simple functions. We therefore obtain the instantaneous power delivered 
by the current in (14) by applying (9), 

1 r T/2 
P = lim — I (sin 2 t + sin 2 nt + 2 sin t sin irt) dt 

30 1 Average Power and RMS Values 

We now consider P as the sum of three average values. The average value 
of sin 2 f over an infinite interval is found by replacing sin 2 * by 
(% — % cos 2*); ^ is obviously %. Similarly, the average value of sin 2 irt 
is also %. And the last term can be expressed as the sum of two cosine 
functions, each of which must certainly have an average value of zero. 

j»=y 8 + % = i w 

An identical result is obtained for the periodic current (15). 

Applying this same method to a current function which is the sum of 
several sinusoids of different periods and arbitrary amplitudes, 

»(*) = Iml cos "l* + 4.2 C0S w 2* + • • • + I «lf cos U N* ( 16 ) 

we find the average power delivered to a resistance R, 

i , =y 2 (v + ^ 2 2 + --- + w)fi a?) 

The result is unchanged if an arbitrary phase angle is assigned to each 
component of the current. This important result is surprisingly simple when 
we think of the steps required for its derivation: squaring the current 
function, integrating, and taking the limit. The result is also just plain 
surprising, because it shows that, in this special case of a current such as 
(16), superposition is applicable to power. Superposition is not applicable 
for a current which is the sum of two direct currents, nor is it applicable 
for a current which is the sum of two sinusoids of the same period. 

Drill Problems 

11-3 A sinusoidal current source I, = 1 0/0° A is connected to each of the 
networks described below. Find the average power delivered by the source in 
each case: (a) 2 ft in parallel with ;4 fl; (b) 4 Q in series with a capacitive 
reactance of 2 fi; (c) a current source 5 /90° A (sensed in the same direction as 
I,) in parallel with ;4 Q. 

Ans. -100; 80; 200 W 

11-4 Find the average power delivered to a 12-Q resistor by each of the three 
periodic current waveforms displayed in Fig. 11-6. 

Ans. 96; 144; 216 W 

11-5 In the circuit of Fig. 11-7, find the average power received by the: (a) 
resistor; (b) dependent source; (c) independent source. 

Ans. -188; 35; 153 mW 


-0.2 -0.1 



0.1 0.2 0.3 




Rfl- '1-6 See Drill Probs. 11-4 and 11-7. 

Fig. 11-7 See Drill Prob. 11-5. 

11-6 Determine the (average) power delivered to the series combination 
of a 5-fl resistor and a 10-mH inductor by the voltage: (a) 
20 cos lOOOt - 15 sin lOOOt V; (b) 20 cos lOOOt - 15 sin 500t V; (c) 20 cos 1000* - 
15 sin (lOOOt - 36.9°) V. 

Am. 12.5; 19.25; 19.7 W 


Most of us are aware that the voltage available at the power outlets in 
our homes is a sinusoidal voltage having a frequency of 60 Hz and a 
"voltage" of 115 V. But what is meant by "115 volts"? This is certainly 
not the instantaneous value of the voltage, for the voltage is not a constant. 
The value of 115 V is also not the maximum value which we have been 
symbolizing as V m ; if we displayed the voltage waveform on a calibrated 
cathode-ray oscilloscope, we should find that the maximum value of this 
voltage at one of our ac outlets is 115\/2 or 162.6 V. We also cannot 
fit the concept of an average value to the 115 V because the average value 
of the sine wave is zero. We might come a little closer by trying the 

303 Avwvfl* Power and RMS Value* 

magnitude of the average over a positive or negative half cycle; by using 
a rectifier-type voltmeter at the outlet, we should measure 103.5 V. As 
it turns out, however, the 115 V is the effective value of this sinusoidal 
voltage. This value is a measure of the effectiveness of a voltage source 
in delivering power to a resistive load. 

Let us now proceed to define the effective value of any periodic 
waveform representing either a current or voltage. We shall consider the 
sinusoidal waveform as only a special, albeit practically important, case. 
Let us arbitrarily define effective value in terms of a current waveform, 
although a voltage could equally well be selected. The effective value of 
any periodic current is equal to the value of the direct current which, 
flowing through a resistance R, delivers the same power to A as the periodic 
current does. In other words, we allow the given periodic current to flow 
through an arbitrary resistance it, determine the instantaneous power i 2 R, 
and then find the average value of i 2 R over a period; this is the average 
power. We then cause a direct current to flow through this same resistance 
and adjust the value of the direct current until the same value of average 
power is obtained. The magnitude of the direct current is equal to the 
effective value of the given periodic current. 

The general mathematical expression for the effective value of i(t) is 
now easily obtained. The average power delivered to the resistor by the 
periodic current i(t) is 

1 r T R r T 

where the period of »(t) is T. The power delivered by the direct current 

P = PR = I.„*R 

Equating the power expressions and solving for I eff , 

*«r = Jif i2dt < 18 > 

v l o 

The result is independent of the resistance R, as it must be to provide us 
with a worthwhile concept. A similar expression is obtained for the effec- 
tive value of a periodic voltage by replacing i and I eff by v and V eff , 

Notice that the effective value is obtained by first squaring the time 
function, then taking the' average value of the squared function over a 
period, and finally taking the square root of the average of the squared 
function. In abbreviated language, the operation involved in finding an 

304 Sinusoidal Analysis 

effective value is the (square) root of the mean of the square; for this reason, 
the effective value is often called the root^nean-square value, or simply 
the rms value. 

The most important special case is that of the sinusoidal waveform. 
Let us select the sinusoidal current 

i(t) = I m cos (at - 9) 

which has a period 

T = — 


and substitute into (18) to obtain the effective value 

y IJ cos* (at- 6) dt 

Thus the effective value of a sinusoidal current is a real quantity which 
is independent of the phase angle and numerically equal to 0.707 times its 
maximum value. A current y/2 cos (ut — 6), therefore, has an effective 
value of 1 A and will deliver the same power to any resistor as will a direct 
current of 1 A. 

The use of the effective value also simplifies slightly the expression for 
the average power delivered by a sinusoidal current or voltage. For 
example, the average power delivered to a resistance R by a sinusoidal 
current is 

p = YJJR 

If we replace I m by V2 I eff , the average power may be written 

P = V* (19) 

The other familiar power expressions may also be written in terms of 
effective values: 

P=V eff I eff cos6 (20) 

V 2 

and p = it (2D 

305 Averag* Power and RMS Values 

The fact that the effective value is defined in terms of an equivalent dc 
quantity provides us with average power formulas for resistive circuits 
which are identical with those used in dc analysis. 

Although we have succeeded in eliminating the factor of one-half from 
our average-power relationships, we must now take care to determine 
whether a sinusoidal quantity is expressed in terms of its maximum value 
or its effective value. In practice, the effective value is usually used in 
the fields of power transmission or distribution and of rotating machinery; 
in the areas of electronics and communications, the maximum value is more 
often used. We shall assume that the maximum value is specified unless 
the term rms is explicitly used. 

In the sinusoidal steady state, phasor voltages and currents may be given 
as either effective values or maximum values; the two expressions differ 
only by a factor \/2. The voltage 50 /30° V is expressed in terms of a 
maximum value; as an rms voltage, we should write 35.35 /30° V rms. 

In order to determine the effective value of a periodic or nonperiodic 
waveform which is composed of the sum of a number of sinusoids of 
different frequencies, we may use the appropriate average power rela- 
tionship (17) developed in the previous section, rewritten in terms of the 
effective values of the several components, 

* = (W + W+ ••■ + W 2 ) R (22) 

These results indicate that if a sinusoidal current of 5 A rms at 60 Hz flows 
through a 2-Q resistor, an average power of 50 W is absorbed by the 
resistor; if a second current, say 3 A rms at 120 Hz, is also present, the 
absorbed power is 68 W; however, if the second current is also at 60 Hz, 
then the absorbed power may have any value between 8 and 128 W, 
depending on the relative phase of the two current components. 

We therefore have found the effective value of a current which is 
composed of any number of sinusoidal currents of different frequencies, 

l e,l = VW + W+ ••• + W (23) 

The total current may or may not be periodic; the result is the same. The 
effective value of the sum of the 60- and 120-Hz currents in the example 
above is 5.83 A; the effective value of the sum of the two 60-Hz currents 
may have any value between 2 and 8 A. 

Drill Problems 

1 1 -7 Find the effective values of the three periodic current waveforms shown 
in Fig. 11-6. 

Ans. 2.83; 3.46; 4.24 A 

306 Sinusoidal Analysis 

1 1-8 Find the effective value of: (a) 2 cos (1000* + 0.1«r) - sin (1000* - 0.15V) V; 
(fc) 2 cos 1000* + sin (500/ + 0.2w) V; (c) c = 1.2 V for < t < 2 ms, 2.4 V for 
2 < f < 4 ms, 3.0 V for 4 < £ < 5 ms, where T = 5 ms. 

Ans. L98; 2J6; 2.24 V 


Historically, the introduction of the concepts of apparent power and power 
factor can be traced to the electric-power industry, where large amounts 
of electrical energy must be transferred from one point to another; the 
efficiency with which this transfer is effected is related directly to the cost 
of the electrical energy, which is eventually paid by the consumer. A 
customer who provides a load which results in a relatively poor transmission 
efficiency must pay a greater price for each kilowatthour (kWh) of electrical 
energy he actually receives and uses. In a similar way, a customer who 
requires a costlier investment in transmission and distribution equipment 
by the power company will also pay more for each kilowatthour. 

Let us first define apparent power and power factor and then show 
briefly how these terms are related to the economic situations mentioned 
above. We shall assume that the sinusoidal voltage 

o = V m cos (at + a) 
is applied to a network, and the resultant sinusoidal current is 

i = I m cos(at + 0) 

The phase angle by which the voltage leads the current is therefore 

8 = a -/? 

The average power delivered to the network, assuming a passive sign 
convention at its input terminals, may be expressed either in terms of the 
maximum values, 

or in terms of the effective values, 

If our applied voltage and current responses had been dc quantities, the 
average power delivered to the network would have been given simply 

307 Average Power and RMS Values 

by the product of the voltage and the current. Applying this dc technique 
to the sinusoidal problem, we should obtain a value for the absorbed power 
which is "apparently" given by the product V eff I eff . This product of the 
effective values of die voltage and current is not the average power; we 
define it as the apparent power. Dimensionally, apparent power must be 
measured in the same units as real power, since cos is dimensionless, but 
in order to avoid confusion the term voltamperes, or VA, or kVA is applied 
to apparent power. Since cos 6 cannot have a magnitude greater than unity, 
it is evident that the magnitude of the real power can never be greater 
than the magnitude of the apparent power. 

Apparent power is not a concept which is limited to sinusoidal forcing 
functions and responses. It may be determined for any current and voltage 
waveshape by simply taking the product of the effective values of the 
current and voltage. This extension of the definition of apparent power 
need not concern us now, but it will receive further amplification in 
connection with general periodic functions when Fourier analysis is dis- 
cussed in Chap. 17. 

The ratio of the real or average power to the apparent power is called 
the power factor, symbolized by PF. Hence, 

average power 

apparent power \„l e „ 

In the sinusoidal case, the power factor is simply cos 6, where is the angle 
by which the voltage leads the current. This relationship is the reason why 
the angle is often referred to as the PF angle. 

For a purely resistive load, the voltage and current are in phase, 9 is 
zero, and the PF is unity. The apparent power and the average power 
are equal. A unity PF, however, may also be achieved for loads which 
contain both inductance and capacitance if the element values and the 
operating frequency are selected to provide an input impedance having 
a zero phase angle. 

A purely reactive load, that is, one containing no resistance, will cause 
a phase difference between the voltage and current of either plus or minus 
90°, and the PF is therefore zero. 

Between these two extreme cases there are the general networks for 
which the PF can range from zero to unity. A PF of 0.5, for example, 
indicates a load having an input impedance with a phase angle of either 
60° or —60°; the former describes an inductive load, since the voltage 
leads the current by 60°, while the latter refers to a capacitive load. The 
ambiguity in the exact nature of the load is resolved by referring to a leading 
PF or a lagging PF, the term leading or lagging referring to the phase 
of the current with respect to the voltage. Thus, an inductive load will have 
a lagging PF and a capacitive load a leading PF. 

308 Sinusoidol Analysis 

The practical importance of these new terms is shown by the several 
examples which follow. Let us first assume that we have a sinusoidal ac 
generator, which is a rotating machine driven by some other device whose 
output is a mechanical torque such as a steam turbine, an electric motor, 
or an internal-combustion engine. We shall let our generator produce an 
output voltage of 200 V rms at 60 Hz. Suppose now that an additional 
rating of the generator is stated as a maximum power output of 1 kW. 
The generator would therefore be capable of delivering an rms current 
of 5 A to a resistive load. If, however, a load requiring 1 kW at a lagging 
power factor of 0.5 is connected to the generator, then an rms current 
of 10 A is necessary. As the PF decreases, greater and greater currents 
must be delivered to the load if operation at 200 V and 1 kW is maintained. 
If our generator were correctly and economically designed to furnish safely 
a maximum current of 5 A, then these greater currents would cause un- 
satisfactory operation. The rating of the generator is more informatively 
given in terms of apparent power in volt-amperes. Thus a 1000-VA rating 
at 200 V indicates that the generator can deliver a maximum current of 
5 A at rated voltage; the power it delivers depends on the load, and in 
an extreme case might be zero. An apparent power rating is equivalent 
to a current rating when operation is at a constant voltage. 

When electric power is being supplied to large industrial consumers 
by a power company, the company will frequently include a PF clause 
in its rate schedules. Under this clause, an additional charge is made to 
the consumer whenever his PF drops below a certain specified value, usually 
about 0.85 lagging. Very little industrial power is consumed at leading 
PFs because of the nature of the typical industrial loads. There are several 
reasons that force the power company to make this additional charge for 
low PFs. In the first place, it is apparent that larger current-carrying 
capacity must be built into its generators in order to provide the larger 
currents that go with lower PF operation at constant power and constant 
voltage. Another reason is found in the increased losses in its transmission 
and distribution system. 

As an example, let us suppose that a certain consumer is using an 
average power of 11 kW at unity PF and 220 V rms. We may also assume 
a total resistance of 0.2 Q in the transmission lines through which the power 
is delivered to the consumer. An rms current of 50 A therefore flows in 
the load and in the lines, producing a line loss of 500 W. In order to supply 
11 kW to the consumer, the power company must generate 11.5 kW (at 
the higher voltage, 230 V). Since the energy is necessarily metered at the 
location of each consumer, this consumer would be billed for 95.6 per cent 
of the energy which the power company actually produced. 

Now let us hypothesize another consumer, also requiring 11 kW, but 
at a PF angle of 60° lagging. This consumer forces the power company 
to push 100 A through his load and (of particular interest to the company) 

309 Average Power and RMS Values 

through the line resistance. The line losses are now found to be 2 kW, 
and the customer's meter indicates only 84.6 per cent of the actual energy 
generated. This figure departs from 100 per cent by more than the power 
company will tolerate; this costs it money. Of course, the transmission losses 
might be reduced by using heavier transmission lines which have lower 
resistance, but this costs more money too. The power company's solution 
to this problem is to encourage operation at PFs which exceed 0.9 lagging 
by offering slightly reduced rates and to discourage operation at PFs which 
are less than 0.85 lagging by invoking increased rates. 

The power drawn by most homes is used at reasonably high PFs (and 
reasonably small power levels); no charge is customarily made for low PF 

Besides paying for the actual energy consumed and for operation at 
excessively low PFs, industrial consumers are also billed for inordinate 
demand. An energy of 100 kWh is delivered much more economically as 
5 kW for 20 h than it is as 20 kW for 5 h, particularly if everyone else 
demands large amounts of power at the same time. 

Drill Problem 

11-9 Determine the PF associated with a load: (a) consisting of a 6.25-/xF 
capacitor in parallel with the series combination of 400-fi resistance and 1 H at 
(o = 400 rad/s; (b) that is inductive and draws 33 A rms and 6.9 kW at 230 V 
rms; (c) composed of parallel loads, one of which draws 10 kVA at 0.8 PF lagging 
and the other 8 kVA at 0.9 PF leading. 

Arts. 0.707 lead; 0.909 lag; 0.985 lag 


Some simplification in power calculations is achieved if power is considered 
to be a complex quantity. The magnitude of the complex power will be 
found to be the apparent power, and the real part of the complex power 
will be shown to be the (real) average power. The new quantity, the 
imaginary part of the complex power, we shall call reactive power. 

We define complex power with reference to a general sinusoidal voltage 
V'ff — V eff/Qy across a pair of terminals and a general sinusoidal current 
W — hff/Oj flowing into one of the terminals in such a way as to satisfy 
the passive sign convention. The average power P absorbed by the two- 
terminal network is thus 

P=V eff I eff cos («,-»,) 

310 SnotoMal Analysis 

Complex nomenclature is next introduced by making use of Euler's formula 
in the same way as we did in introducing phasors. We express P as 

P=V eff /,, ff Re[e«»--W] 
or P = Re [V efl ei«"I efl e->«] 

The phasor voltage may now be recognized as the first two factors within 
the brackets in the equation above, but the second two factors do not quite 
correspond to the phasor current because the angle includes a minus sign 
which is not present in the expression for the phasor current. In other 
words, the phasor current is 

W = *.«•"* 

and we therefore must make use of conjugate notation, 

l eff — l eifi 


P=Re(V eff i; ff ) 

and we may now let power become complex by defining the complex power 
P as 

P = W, (24) 

If we first inspect the polar or exponential form of the complex power 

r — Vetthffi 

it is evident that the magnitude of P is the apparent power, and the angle 
of P is the PF angle, that is, the angle by which the voltage leads the 
current. In rectangular form, 

P = P + /«? (25) 

where P is the real average power, as before. 1 The imaginary part of the 
complex power is symbolized as Q and is termed the reactive power. The 
dimensions of Q are obviously the same as those of the real power P, the 

'It should be noted that P is not the magnitude of P, although such nomenclature has been used 
previously. For example, V t „ is the magnitude of V,,,, Z L is the magnitude of Z t , and 
so forth. 



Fig. 11-8 The current phasor l eff is resolved into two components, one in 
phase with the voltage phasor \ eff and the other 90° out of phase with the 
voltage phasor. This latter component is called a quadrature component. 

complex power P, and the apparent power |P|. In order to avoid confusion 
with these other quantities, the units of Q are defined as vars, standing 
for voltamperes reactive. From (24), it is seen that 

Another interpretation of the reactive power may be seen by constructing 
a phasor diagram containing \ eff and \ eff , as shown in Fig. 11-8. If the 
phasor current is resolved into two components, one in phase with the 
voltage, having a magnitude I eff cos(0 v — { ), and one 90° out of phase 
with the voltage, with magnitude I eff sin (0 V — 6 t ), then it is clear that the 
real power is given by the product of the magnitude of the voltage phasor 
and the component of the phasor current which is in phase with the 
voltage. Moreover, the product of the magnitude of the voltage phasor 
and the component of the phasor current which is 90° out of phase with 
the voltage is the reactive power Q. It is common to speak of die compo- 
nent of a phasor which is 90° out of phase with some other phasor as a 
quadrature component. Thus Q is simply V eff times the quadrature compo- 
nent of l eff ; Q is also known as the quadrature power. 

The sign of the reactive power characterizes the nature of a passive 
load at which \ eff and I eff are specified. If the load is inductive, then ff v — i 
is an angle between and 90°, the sine of this angle is positive, and the 
reactive power is positive. A capacitive load results in a negative reactive 

Just as a wattmeter 2 reads the average real power drawn by a load, 
a varmeter will read the average reactive power Q drawn by the load. 
Both quantities may be metered simultaneously. In addition, watthour- 

2 The wattmeter is discussed in Sec. 12-5. 






I 1 ' 


I 1 * 




Fig. 11-9 A circuit used to show that the complex power drawn by two 
parallel loads is the sum of the complex powers drawn by the individual loads. 

meters and varhour-meters may be used simultaneously to record real and 
reactive energy used by any consumer during any desired time interval. 
From these records the average PF may be determined and the consumer's 
bill may be adjusted accordingly. 

It is easy to show that the complex power delivered to several inter- 
connected loads is the sum of the complex powers delivered to each of 
the individual loads, no matter how the loads are interconnected. For 
example, consider the two loads shown connected in parallel in Fig. 11-9. 
If rms values are assumed, the complex power drawn by the combined 
loads is 

and thus 

p = vr = \(i x + 1 2 )' = v(i* + 1 2 *) 

p = Wl\ + VIj 

as stated. 

These new ideas can be clarified by a practical numerical example. 
Let us suppose that an industrial consumer is operating a 1-kW induction 
motor at a lagging PF of 0.8. In order to obtain lower electrical rates, 
he wishes to raise his PF to 0.95 lagging. Although the PF might be raised 
by increasing his real power and maintaining the reactive power constant, 
this would not result in a lower bill; this cure therefore does 'not interest 
the consumer. A purely reactive load must be added to the system, and 
it is clear that it must be added in parallel, since the supply voltage to 
the induction motor must not change. The circuit of Fig. 11-9 is thus 
applicable if we interpret P 1 as the induction motor power and P 2 as the 
complex power drawn by the corrective device. Let us assume a voltage 
of 200/0° V rms. 

The complex power supplied to the induction motor must have a real 
part of 1000 W and an angle of cos -1 (0.8). Hence, 

100 0/cos- 1 (0.8) 


= 1000 + /750 


313 Average Power and RMS Values 

In order to achieve a PF of 0.95, the total complex power must become 

p _ 100 ° /cos- 1 (0.95) = 1000 + ;329 

Thus, the complex power drawn by the corrective load is 

P 2 = -/421 

The necessary load impedance Z 2 may be found in several simple steps. 
The current drawn by Z 2 is 

ll = h = ^L = * 

* 2 V 200 


I 2 = /2.105 

and, therefore, 

z V 200 
2 I 2 /2.105 


= -/95.0 a 

If the operating frequency is 60 Hz, this load can be provided by a 27.9-jliF 
capacitor. The load may also be simulated by a synchronous capacitor, 
a type of rotating machine, although this is usually economical only for 
much smaller capacitive reactances. Whatever device is selected, its initial 
costs, maintenance, and depreciation must be covered by the reduction in 
the electric bill. 

Drill Problem 

11-10 Find the value of an impedance which: (a) absorbs a complex power of 
460 0/30° VA at 230 V rms; (b) absorbs a complex power of 500 0/45° VA when 
the rms current through it is 12.5 A; (c) requires — 1500 vars at 230 V rms and 10 A 

Ans. 9.95 + f'5.75; 17.4 - jlS.0; 22.6 + J22.6 a 


□ 1 For the circuit shown in Fig. 11-10, determine the instantaneous powers de- 
livered to the resistor if v s = : (a) 30 cos 2500f V; (b) 30u(t) V; (c) 30 cos 2500* + 
30m(«) V. 




Fig. 1J-10 See Prob. 1. 

D 2 The current through a 50-fl resistor is given as t = 3e~ 2 ' A for t > and t = 
for t < 0. Find the average power delivered to the resistor during the time 
interval: (a) < t < 0.5 s; (b) -0.5 < t < 0.5 s; (c) < t < 5 s. 

□ 3 The voltage u is across the series combination of 6 U and 20 mH. Find the 
average power delivered to this impedance if v = : (a) 10 cos 400t V; (b) 10 sin 400t 
V; (c) 10 sin (400f + 20°) V; (d) 6 + 10 cos 400f V. 

□ 4 Find Rj and |I 8 | in the circuit shown in Fig. 11-11 if the average power 
delivered to each resistor is 1.5 W. 

48 Q 

b) = 200 rad / s 

: h 

Fig. 11-11 See Prob. 4. 

□ 5 Find the average power delivered to the 3-fl resistor in the circuit shown in 
Fig. 11-12. 

Fig. 11-12 See Prob. 5. 

□ 6 Assume a Thevenin equivalent source composed of V s in series with Z eg = 
fi e9 + jX eq . (a) Prove that maximum average power is delivered to a load 
% L = R L + jX L when R L = R e gandX L = — X eq . (b) Prove that maximum average 
power is delivered to a load R L when R L = \"Z elJ \. 

□ 7 The Thevenin equivalent of a sinusoidal voltage source is the ideal voltage 

315 Avarag* Power and RMS Values 

source v s = V m cos cot in series with a resistance R eg . (a) What is the maximum 
power that can be delivered to an external load resistance? (b) If the source has 
an internal impedance Z eg = R eq + jX eq , what is the maximum power that can 
be delivered to an external load impedance? 

□ 8 An ideal voltage source, 100 /0° V, is in series with a 20042 resistor and a 
capacitive reactance of —100 ft. (a) What impedance Z L in parallel with the 
capacitance will absorb maximum average power, and what is this maximum 
power? (b) What resistive load R L in parallel with the capacitance will absorb 
maximum average power, and what is this maximum power? 

□ 9 Find the effective value of each of the following voltages: (a) 20 cos 800* V; 
(b) 20 cos (800* + 20°) V; (c) 12 cos (800* + 20°) + 16 cos (SOOt - 70°) V; (d) 

4 cos (800* + 20°) + 12 V2~ cos (800* + 65°); (e) 15 cos 800* + 10 sin 801* - 

5 V3 sin 802* V. 

D 10 Find the effective value of the periodic voltage v if: v = 2, < * < 4; 
v = * - 2, 4 < * < 10; T = 10. 

Dll A current waveform is / for a time *j and then kl for a like time. If the 
period is 2* lt determine k such that the effective value is 2I . 

D 1 2 Let i = 4 - 8[u(t - 2) - u(* - 3)] + tu(t - 2) for a period interval 
< t < 5. For this current, determine: (a) the positive and negative peak values; 
(b) the average value; (c) the effective value. 

D 13 A resistance R and reactance X in series are connected to a 115-V 60-Hz 
voltage supply. Good laboratory instruments are used to show that the reactor 
voltage is 75 V and the total power supplied to the circuit is 190 W. Find R, 
X, and the rms current. 

□ 14 With reference to the circuit of Fig. 11-13, what should be the value of R L 
to absorb a maximum power? Find the value of this maximum power. 

Fig. 11-13 See Prob. 14. 

□ 15 In the circuit shown in Fig. 11-14, I L = 12 A rms and I s = 15 A rms. Find 
the average power delivered to the resistor without knowing the value of co. 

□ 16 The PF of the total load supplied by the current source of Fig. 11-14 is 0.5 
lagging. What is the operating frequency in radians per second? 

Fig. 11-14 See Probs. 15, 16, and 17. 

D 17 The operating frequency of the circuit shown in Fig. 11-14 is 1000 rad/s. 
Find the real, reactive, and apparent power supplied by the source if I s = 
2.6 /12° A rms. 

□ 18 A source, 120 V rms at 60 Hz, supplies 2400 VA to a load operating at a 
0.707 lagging PF. Find the value of capacitance and its necessary kilovoltampere 
rating such that the PF will be raised to 0.95 lagging when it is placed in parallel 
with the load. 

□ 19 Three parallel loads drawing 3 kW, 5kVA at 0.866 PF lagging and 4 kVA at 
0.707 PF lagging are connected to a 230-V 60 Hz source. How many kilovolt- 
amperes are required by the total load? 

□ 20 A voltage source, 40 /20° V, is in series with an impedance % x and the parallel 
combination of impedances Z 2 and Z 3 . Find the complex power delivered to every 
impedance if: (a) Z x = /10 fi, Zj = 6 Q, Z 3 = -/8 Q; (6) Z 1 = 3 + /4 Q, 
Z 2 = 2 - ;'4 Q, Z 3 = 1 + /8 Q. 

□ 21 The voltage across a device is labeled V and the current entering the 
plus-marked terminal is I. The complex power delivered to the device is P, and 
<j = 10 3 rad/s. (a) If V = 2 - ;6 V and P = 20 - ;10 VA, determine two passive 
series elements that are equivalent to the device, (b) If I = 3 + ;3 A and 
P = 20 + ;40 VA, determine two passive parallel elements that are equivalent 
to the device. 

□ 22 Three passive loads, Zj, Z 2 , and Z 3 , are receiving the complex power values, 
2 + ;3, 3 — /l.andl + /2 VA, respectively. What total complex power is received 
if the three loads are: (a) in series with a voltage source 100 /30° V; (b) in parallel 
with a current source 1200 /— 17° A? 


Paty pha i c Circuitiy 









One of the reasons for studying the sinusoidal steady state is that roost 
household and industrial electric power is utilized as alternating curwntf ? 
The sinusoidal waveform may characterize a special matheBttatk^fuiQcCio%, 
but it represents a very common and very useful fordt^ functtojb^^, 
polyphase source is even more specialized, but we again consider it beekfeSjtr-: 
almost the entire output of the electric power industry in this cewjtkfy&i, 
generated and distributed as polyphase power at a 60-Hz frecpieney . Bdra%$: : ;j 
defining our terms carefully, let us look briefly at the most common peSy*.' 
phase system, a balanced three-phase system. The source has perhaps thre«£ 




318 Sinusoidal Analysis 

terminals, and voltmeter measurements will show that sinusoidal voltages 
of equal magnitude are present between any two terminals. However, these 
voltages are not in phase; it will be easily shown later that each of the 
three voltages is 120° out of phase with each of the other two, the sign 
of the phase angle depending on the sense of the voltages. A balanced 
load draws power equally from the three phases, but when one of the 
voltages is instantaneously zero, the phase relationship shows that the other 
two must each be at half amplitude. At no instant does the instantaneous 
power drawn by the total load reach zero; as a matter of fact, this total 
instantaneous power is constant. This is an advantage in rotating machin- 
ery, for it keeps the torque much more constant than it would be if a 
single-phase source were used. There is less vibration. 

There are also advantages in using rotating machinery to generate 
three-phase power rather than single-phase power, and there are economi- 
cal advantages in favor of the transmission of power in a three-phase 

The use of a higher number of phases, such as 6- and 12-phase systems, 
is limited almost entirely to the supply of power to large rectifiers. Here, 
the rectifiers convert the alternating current to direct current, which is 
required for certain processes such as electrolysis. The rectifier output is 
a direct current plus a smaller pulsating component, or ripple, which 
decreases as the number of phases increases. 

Almost without exception, polyphase systems in practice contain sources 
which may be closely approximated by ideal voltage sources or by ideal 
voltage sources in series with small internal impedances. Three-phase 
current sources are extremely rare. 

It is convenient to describe polyphase voltages and currents using a 
double-subscript notation. With this notation, a voltage or current, such 
as V a6 or I aA , has more meaning than if it were indicated simply as V 3 
or l x . By definition, let the voltage of point a with respect to point b be 
\ ab . Thus, the plus sign is located at a, as indicated in Fig. 12-la. With 
reference to Fig. 12-lfo, it is now obvious that \ ad = \ ab + Y cd . The power 
of the double-subscript notation lies in the fact that Kirchhoff 's voltage 

Fia. 12-1 (a) The definition of the voltage V a ,. (fc] V ad = \ ab + V te + 

"at ~ "a& + "at- 


' *, 1 100 £120° V 


ioo /-i2o °vy ioo (o° v 


Fig. 12-2 A network used as a numerical example of double-subscript 
voltage notation. 

law requires the voltage between two points to be the same, regardless 
of the path chosen between the points, and thus V ad — \ ab + V,^ = 
V ac + V cd = V ai) + V bc + V c(j , etc. It is apparent that Kirchhoff's voltage 
law may be satisfied without reference to the circuit diagram; correct 
equations may be written even though a point, or subscript letter, is 
included which is not marked on the diagram. For example, we might 
also have written, above, \ ai — \ ax + V zd . 

One possible representation of a three-phase system of voltages 1 will 
be found to be that of Fig. 12-2. Let us assume that the voltages V an , %„, 
and \ m are known, 

V a „ = 100/0° V rms 
Van = 100 /- 120° 
V cn = 100 /-240° 

and thus the voltage V a6 may be found, with an eye on the subscripts, 

'aft = 'an ' *nb ~ *an ~ 'ftn 

= 100/0° - 100 /- 120° 
= 100 - (-50 - /86.6) 
= 173.2 /30° 

The three given voltages and the construction of the phasor \ ab are shown 
on the phasor diagram of Fig. 12-3. 

A double-subscript notation may also be applied to currents. We define 
the current l ab as the current flowing from a to b by the direct path. In 
every complete circuit we consider, there must of course be at least two 
possible paths between the points a and b, and we agree that we shall not 
use double-subscript notation unless it is obvious that one path is much 

'Bms values of currents and voltages will be used throughout this chapter. 


V.5 = X a „ + \ nb 

Fig. 12-3 This phasor diagram illustrates the graphical use of the double- 
subscript voltage convention to obtain V a6 for the network of Fig. 1 2-2. 

shorter, or much more direct. Usually this path is through a single element. 
Thus, the current I ab is correctly indicated in Fig. 12-4, but the mere 
identification of a current as l cd would cause confusion. 

Before considering polyphase systems, we shall make use of double- 
subscript notation to help with the analysis of a special single-phase system. 


v b*(T) 



Fig. 12-4 An illustration of the use and misuse of the double-subscript 
convention for current notation. 

Drill Problems 

1 2-1 Given that V 12 = 6 /30° , V 23 = 2/01, V 24 = 6 /-60" , and V 15 = 4/901, 
find: (a) V 14 j (b) V 43 ; (c) V 35 . 

Ans. 5.29 /100.9° ; 7.26 /172.1" ; 8.48 / -15° 

Fig. 12-5 See Drill Prob. 12-2. 

o.i n . 


20/180°/ , 


i a 

0.2 n 


N 5^-/10 Ji 



321 Polyphase Circuits 

T2-2 In the circuit shown in Fig. 12-5, determine: (a) I„ N ; (b) I AN ; (c) I AB . 

Ans. 0; 8 / -90° ; 21.5 /21.8° A 

Fig. 12-c* (a) A single-phase three-wire source, [b] The representation of a 
single-phase three-wire source by two identical voltage sources. 

Single -phase 





-o b 



A single-phase three-wire source is defined as a source having three output 
terminals, such as a, n, and b in Fig. 12-6a, at which the phasor voltages 
V an and V ni) are equal. The source may therefore be represented by the 
combination of two identical voltage sources; in Fig. 12-6b, \ an = V n4 = 
Vj. It is apparent that \ ab = 2\ an = 2V nb , and we therefore have a source 
to which loads operating at either of two voltages may be connected. The 
normal household system is single-phase three-wire, permitting the opera- 
tion of both 115-V and 230-V appliances. The higher- voltage appliances 
are normally those drawing a larger power, and thus they cause a current 
in the lines which is only half that which operation at the same power 
and half the voltage would produce. Smaller-diameter wire may con- 
sequently be used safely in the appliance, the household distribution system, 
and the distribution system of the utility company. 

The name single phase arises because the voltages \ an and \ nb , being 
equal, must have the same phase angle. From another viewpoint, however, 
the voltages between the outer wires and the central wire, which is usually 
referred to as the neutral, are exactly 180° out of phase. That is, \ an = 
— Vfc, and V„ B + V^, = 0. In a following section we shall see that balanced 
polyphase systems are characterized by possessing a set of voltages of equal 
magnitude whose (phasor) sum is zero. From this viewpoint, then, the 
single-phase three-wire system is really a balanced two-phase system. "Two 
phase," however, is a term that is traditionally reserved for a relatively 
unimportant system utilizing two voltage sources 90° out of phase; we shall 
not discuss it further. 

Let us now consider a single-phase three-wire system which contains 
identical loads Z p between each outer wire and the neutral (Fig. 12-7). 

Fig. 12-7 A simple single-phase three-wire system, 
identical and the neutral current is zero. 

The two loads are 

We shall first assume that the wires connecting the source to the load are 
perfect conductors. Since 


and, therefore, 

V V 

j an j nb 

l aA ~~ 7 ~~ Bb ~ 7 

I n W — 1.8(1 + *Aa — *Bb *aA ~ " 

Thus there is no current in the neutral wire, and it could be removed 
without changing any current or voltage in the system. This result is 
achieved through the equality of the two loads and of the two sources. 

We next consider the effect of a finite impedance in each of the wires. 
If lines aA and bB each have the same impedance, this impedance may 
be added to Z p , resulting in two equal loads once more and zero neutral 
current. Now let us allow the neutral wire to possess some impedance Z„. 
Without carrying out any detailed analysis, superposition should show us 
that the symmetry of the circuit will still cause zero neutral current. 
Moreover, the addition of any impedance connected directly from one of 
the outer lines to the other outer line also yields a symmetrical circuit and 
zero neutral current. Thus, zero neutral current is a consequence of a 
balanced, or symmetrical, load; any impedance in the neutral wire does 
not destroy the symmetry. 

The most general single-phase three-wire system will contain unequal 
loads between each outside line and the neutral and another load directly 
between the two outer lines; the impedances of the two outer lines may 
be expected to be approximately equal, but the neutral impedance may 
be slightly larger. An example of such a system is shown in Fig. 12-8. 
The analysis of the circuit may be achieved by assigning mesh currents 




ns or, 

Vnns V- 


'50 n 

■ N 

115 10'( + 
Vnns V-. 





in » 

Fig. 1 2-8 A typical single-phase three-wire system, 

and writing the appropriate equations. The results of this labor are 

Ij = 11.2 /- 19.8° A rms 

1 2 = 9.38 /-24.5 

1 3 = 10.4 /-21.8° 

The currents in the outer lines are thus 

l aA = I, = 11.2 /- 19.8° A rms 
Iw. = -I 3 = 10-4 /158.2° 

and the smaller neutral current is 

I»w = I 3 - I 4 = 0-95 /- 177.9° A rms 

The power drawn by each load may be determined, 

P50 = III - I 2 I 2 (50) = 207 W 

which could represent two 100-W lamps in parallel, 

which might represent one 100-W lamp, 

'wflo = Il 2 l 2 (20) = 1763 W 

which we may think of as a 2-hp induction motor. The total load power 
is 2087 W. The loss in each of the wires is next found: 


Fig. 1 2-9 The source voltages and three of the currents in the circuit of 
Fig. 12-8 are shown on a phasor diagram. Note that X aA + l bB + I TtN — 0. 

Ka = IW) = 126 W 
*» = tl 3 l 2 (l) = 108 W 

Pun = IUi 2 (3) = 2.7 W 

or a total line loss of 237 W. The wires are evidently quite long; otherwise, 
the relatively high power loss in the two outer lines would cause a dan- 
gerous temperature rise. The total generated power must therefore be 
2324 W, and this may be checked by finding the power delivered by each 
voltage source: 

P an = 115(11.2)005 19.8° = 1218 W 

P^ = 115(10.4) cos 21.8° = 1108 W 

or a total of 2326 W. The transmission efficiency for this system is 



2087 + 237 

This value would be unbelievable for a steam engine or an inter- 
nal-combustion engine, but it is too low for a well-designed distribution 
system. Larger-diameter wires should be used if the source and the load 
cannot be placed closer to each other. 

A phasor diagram showing the two source voltages, the currents in the 
outer lines, and the current in the neutral is constructed in Fig. 12-9. The 
fact that l aA + l iB + L.JV = is indicated on the diagram. 

Drill Problem 

1 2-3 Replace the 50-fi load by a 10-fi load in the circuit shown in Fig. 12-8, 
and then find the average power delivered to the: (a) 10-fi load; (b) 100-fl load; 
(c) 20 + /10-fi load. 

Ans. 157; 623; 1670 W 


325 Polyphasa Circuits 


Three-phase sources have three terminals, called the line terminals, and 
they may or may not have a fourth terminal, the neutral connection. We 
shall begin by discussing a three-phase source which does have a neutral 

Fig. 12-10 A Y-connected three-phase source. 

connection. It may be represented by three ideal voltage sources connected 
in a Y, as shown in Fig. 12-10; terminals a, b, c, and n are available. We 
shall consider only balanced three-phase sources which may be defined as 

IV..I = |VJ = IVJ 
and V a „ + V,, + V„, = 

These three voltages, each existing between one line and the neutral, are 
called phase voltages. If we arbitrarily choose V an as the reference, 

v., = v p /oi 

where we shall consistently use V p to represent the rms magnitude of any of 
the phase voltages, then the definition of the three-phase source indicates 
that either 

V^ = y-120- V c „ = V-240° 
or V^ = V p /1201 V c „ = V2401 

The former is called positive phase sequence, or abc phase sequence, and 
is shown in Fig. 12-1 la; the latter is termed negative phase sequence, or 
cba phase sequence, and is indicated by the phasor diagram of Fig. 12-llfc. 
It is apparent that the phase sequence of a physical three-phase source 
depends on the arbitrary choice of the three terminals to be lettered o, 
b, and c. They may always be chosen to provide positive phase sequence, 

\n=V p l=Mt° 

V in =V„Z120° 

(+) sequence 

V,,. = V. & 

( — ) sequence 

V <m =V„Zfi« 

■v p im° 



fig. 1 2-1 1 [a) Positive, or abc, phase sequence, (b) Negative, or cba, 
phase sequence. 

and we shall assume that this has been done in most of the systems we 

Let us next find the line-to-line voltages (or simply "line" voltages) 
which are present when the phase voltages are those of Fig. 12-1 la. It 
is easiest to do this with the help of a phasor diagram, since the angles 
are all multiples of 30° The necessary construction is shown in Fig. 12-12; 
the results are 

V„ b = V3 V30I V^ = V3 V-90° V c „ = V3 V p /-210° 

Kirchhoff's voltage law requires the sum of these three voltages to be zero, 
and it is zero. 

Denoting the magnitude of any of the line voltages by V L , then one 
of the important characteristics of the Y-connected three-phase source may 
be expressed as 

V L = V3 V. 

Rg. 12-12 A phasor diagram which is used to determine the line voltages 
from the given phase voltages. 


Fig. 12-13 

a neutral. 

A balanced three-phase system, connected Y-Y, and including 

Note that, with positive phase sequence, V OB leads V^ and V^ leads \ m , 
in each case by 120°, and also that V a6 leads V^ and V^ leads V co , again 
by 120° . The statement is true for negative sequence if "lags" is substituted 
for "leads." 

Now let us connect a balanced Y-connected three-phase load to our 
source, using three lines and a neutral, as drawn in Fig. 12-13. The load 
is represented by an impedance 7. p between each line and the neutral. 
The three line currents are found very easily, since we really have three 
single-phase circuits which possess one common lead: 

hA = 

V ta V n „/-120° 

h B - z 

L, = W-240° 

= W-120° 

and thus 

*Wn — **A + Iftfl + leC — 

Thus, the neutral carries no current if the source and load are both balanced 
and if the four wires have zero impedance. How will this change if an 
impedance Z t is inserted in series with each of the three lines and an 
impedance Z„ is inserted in the neutral? Evidently, the line impedances 
may be combined with the three load impedances; this effective load is 
still balanced, and a perfectly conducting neutral wire could be removed. 
Thus, if no change is produced in the system with a short circuit or an 
open circuit between n and N, any impedance may be inserted in the 
neutral and the neutral current will remain zero. 

It follows that, if we have balanced sources, balanced loads, and bal- 
anced line impedances, a neutral wire of any impedance may be replaced 
by any other impedance, including a short circuit and an open circuit. 


Fig. 12-14 A balanced three-phase three-wire Y-Y connected system. 

It is often helpful to visualize a short circuit between the two neutral points; 
the problem is then reduced to three single-phase problems, all identical. 
We say that we thus work the problem on a "per-phase" basis. 

Let us work several problems involving a balanced three-phase system 
having a Y-Y connection. A straightforward problem is suggested by the 
circuit of Fig. 12-14; we are asked to find the several currents and voltages 
throughout the circuit and to find the total power. 

Since one of the source phase voltages is given, and since positive phase 
sequence is assumed, the three phase voltages are 

V„„ = 200/0° 

V bn = 200 7-120° V = 2007-240° 

The line voltage is 200 \/3, or 346 V rms; the phase angle of each line volt- 
age can be determined by constructing a phasor diagram, as before. As a 
matter of fact, the phasor diagram of Fig. 12-12 is applicable, and \ ab is 
346/30° V. 

Let us work with phase A. The line current is 

I„. =• 


2/-60" A rms 

Z„ 100/60° 
and the power absorbed by this phase is, therefore, 

P AN = 200(2) cos (0° + 60°) = 200 W 

Thus, the total power drawn by the three-phase load is 600 W. The 
problem is completed by drawing a phasor diagram and reading from it 
the appropriate phase angles which apply to the other line voltages and 
currents. The completed diagram is shown in Fig. 12-15. 

We may also use per-phase methods to work problems in what might 
be called the backward direction. Suppose that we have a balanced 


Fig. 12-15 The phasor diagram that is applicable to the circuit of Fig. 12-14. 

three-phase system with a line voltage of 300 V rms, and we know that 
it is supplying a balanced Y-connected load with 1200 W at a leading PF 
of 0.8. What is the line current and the per-phase load impedance? It 
is evident' that the phase voltage is 300/ V3 V rms and the per-phase power 
is 400 W. Thus the line current may be found from the power relationship 

400 = -?* (I L )(0.8) 

and the line current is therefore 2.89 A rms. The phase impedance is given 

|ZJ= ^ = ^M,60 

Since the PF is 0.8, leading, the impedance phase angle is —36.8°, and 

Z p = 60 / -36.8° 12. 

More complicated loads can be easily handled, since the problems 
reduce to simpler single-phase problems. Suppose that a balanced 600-W 
lighting load is added (in parallel) to the system above. A suitable per-phase 
circuit is first sketched, as shown in Fig. 12-16. 

Fig. 12-16 The per-phase circuit that is used to analyze a balanced 
three-phase example. 

I 2 

►200 W 

400 W 
0.8 P.F. 


330 Sinusoidal Analysis 

The magnitude of the lighting current is determined by 

200= vT |Il|cos0 ° 

and |l t |= 1.155 

In a similar way, the magnitude of the capacitive load current is found 
to be unchanged from its previous value, 

|I 2 | = 2.89 

If we assume that the phase with which we are working has a phase 
voltage with an angle of 0°, then 

Ij = 1.155/0° I 2 = 2.89 7 + 36.8° 
and the line current is 

h = Ii + h = 3.87 /+26.6° A rms 
The power generated by this phase of the source is, therefore, 

P p = -3^3.87 cos ( + 26.6°) =600 W 

which checks with the original hypothesis. 

If an unbalanced Y-connected load is present in an otherwise balanced 
three-phase system, the circuit may still be analyzed on a per-phase basis 
if the neutral wire is present and if it has zero impedance. If either of 
these conditions is not met, other methods must be used. An engineer who 
spends most of his time with unbalanced three-phase systems will find the 
use of symmetrical components a great timesaver. We shall not discuss this 
method here. 

Drill Problems 

1 2-4 A balanced three-phase three-wire system has a Y-connected load contain- 
ing a 50-12 resistor, a 5-fiF capacitor, and a 0.56-H inductor in series in each phase. 
Using positive phase sequence with V an = 39 0/30° V rms and « = 500 rad/s, 
find: («) \ m ; (b) V te ; (c) V„. 

Am. 39 0/150" : 675/0°: 675 / -60" V rms 

331 Polyphase Circuits 

1 2-5 For the circuit described in Drill Prob. 12-4 above, find: (a) l aA ; (b) I hB ; 

(C) he- 

Ans. 3 / -22.6° : 3 /37.4° : 3/97.4° A rms 

1 2-6 A 440- V rms (line voltage) three-phase three-wire system feeds two bal- 
anced Y-connected loads. One load is an induction motor which may be repre- 
sented by an impedance of 10 + /'5 $2 per phase. The other is a lighting load 
equivalent to 15 U per phase. Find the average power: (a) delivered to the lighting 
load; (b) delivered to the induction motor; (c) provided by one phase of the source. 

Ans. 9.46; 12.9; 15.5 kW 

12-7 A balanced three-phase three-wire system supplies two balanced Y- 
connected loads. The first draws 6 kW at 0.8 PF lagging while the other requires 
12 kW at 0.833 PF leading. If the current in each line is 8 A rms, find the cur- 
rent in the: (a) first load; (b) second load; (c) source phase. 

Ans. 3.28; 6.30; 8 A rms 


A three-phase load is more apt to be found A-connected than Y-connected. 
One reason for this, at least for the case of an unbalanced load, is the 
flexibility with which loads may be added or removed on a single phase. 
This is difficult (or impossible) to do with a Y-connected three-wire load. 
Let us consider a balanced A-connected load which consists of an 
impedance Z p inserted between each pair of lines. We shall assume a 
three-wire system for obvious reasons. With reference to Fig. 12-17, let 
us assume known line voltages 

V L = |V.»| = |VJ = |V M 

or known phase voltages 

V, = |V„| = |VJ = |V M 

Fig. 12-17 A balanced A-connected load is present on a three-wire three- 
phase system. The source happens to be Y-connected. 




z p 


332 Sinusoidal Analysis 


V L = V3 V p 


V„ 6 = V3 V a „/301 

and so forth, as before. Since the voltage across each branch of the A is 
known, the phase currents axe found, 

l AB — rj 


In. = 

z„ ""* - z„ 

and their differences provide us with the line currents, such as 

The three phase currents are of equal magnitude, 

h = 11**1 = |I*ol = IhJ 

The line currents are also equal in magnitude. This is due to having phase 
currents which are equal in magnitude and necessarily 120° out of phase. 
The symmetry is apparent from the phasor diagram of Fig. 12-18. We 
thus have 


h = Ha a\ = \h B \ = Hod 

It. = V3 I, 

Let us disregard the source for the moment and consider only the 
balanced load. If the load is A-connected, then the phase voltage and 
the line voltage are indistinguishable, but the line current is larger than the 
phase current by a factor of V3; with a Y-connected load, however, the phase 

Fig. 12-18 A phasor diagram which could apply to the circuit of Fig. 12-17 
if Z p is an inductive impedance. 

+ V BC 

333 Polyphase Circuits 

current and the line current refer to the same current, and the line voltage 
is greater than the phase voltage by a factor of y3. 

The solution of three-phase problems will be speedily accomplished if 
the \/3's are used properly. Let us consider a typical numerical example. 
We are to determine the magnitude of the line current in a 300-V rms 
three-phase system which supplies 1200 W to a A-connected load at a 
lagging PF of 0.8. Let us again consider a single phase. It draws 400 W, 
0.8 lagging PF, at a 300-V rms line voltage. Thus, 

400 = 300(J p )(0.8) 
and J p = 1.667 A rms 

and the relationship between phase currents and line currents yields 

l L = V5 (1.667) = 2.89 A rms 

Furthermore, the impedance in each phase must be 

Z„ = -^ /cos- 1 0.8 = 180/36.8° Q 

Now let us change the statement of the problem: the load is Y-connected 
instead of A-connected. On a per-phase basis, we now have a phase voltage 
of 300/ V^ V rms, a power of 400 W, and a lagging PF of 0.8. Thus, 

400 = ^(V(0.8) 
and I p = 2.89 or I L = 2.89 A rms 

The impedance in each phase of the Y is 

Z r = Jg^ /cos-iQ.8 = 60/36.8° U 

The V§ factor not only relates phase and line quantities but also appears 
in a useful expression for the total power drawn by any balanced three- 
phase load. If we assume a Y-connected load with a power-factor angle 
0, then the power taken by any phase is 

= V p I L cosO 
= —r=I, costf 

334 Sinusoidal Analysis 
and the total power is 

P = 3P„ 

= V5 v L r L cos e 

In a similar way, the power delivered to each phase of a A-connected load 

P,= V„I p cos6 

= V L I p cos6 

= V t -^cos0 

or a total power 

P = 3P„ 


P = y/Z V L I L cos e 


Thus (1) enables us to calculate the total power delivered to a balanced 
load from a knowledge of the magnitude of the line voltage, of the line 
current, and of the phase angle of the load impedance (or admittance). 
The numerical example above can be worked in one line: 

1200 = V3(300)(I t )(0.8) 

I L = -4= = 2.89 A rms 

The source may also be connected in A. This is not typical, however, 
for a slight unbalance in the source phases can lead to large currents 
circulating around the A loop. As an example, let us call the three sin- 
gle-phase sources V ai) , V bc , and \ ci . Before closing the A by connecting 
d to a, let us determine the unbalance by measuring the sum V a6 + Vj, c + 
\ cd . Suppose that the magnitude of the resultant is only 1 per cent of the 
line voltage. The circulating current is thus approximately % per cent of 
the line voltage divided by the internal impedance of any source. How 
large is this impedance apt to be? It must depend on the current that the 
source is expected to deliver with a negligible drop in terminal voltage. 
If we assume that this maximum current causes a 1 per cent drop in the 
terminal voltage, then it is seen that the circulating current is one-third 
of the maximum current. This reduces the useful current capacity of the 
source and also increases the losses in the system. 

335 p olyph<m Circuits 

Drill Problems 

12-8 A balanced three-phase three-wire system has a A-connected load with 
a 50-fi resistor, a 5-|tiF capacitor, and a 0.56-H inductor in series in each phase. 
Using positive phase sequence with V a „ = 390 /30° V rms and <o = 500 rad/s, 
find: (a) I BC ; (b) l aA ; (c) I cC . 

Am. 5.2 0/7.4° : 9 / -142.6° : 9 /97.4° A rms 

12-9 A balanced A-connected load contains 8 + /4 U per phase, while a balanced 
Y-connected load consists of 2 — ;'l fi per phase. Both loads are connected in 
parallel to a three-phase three-wire system in which V L = 120 V rms at the loads. 
The three lines extending from the loads to the source each have a resistance 
of 0.2 Q. Find the total power: (a) delivered to the A-connected load; (b) delivered 
to the Y-connected load; (c) lost in the wires. 

Ans. 1.43; 4.32; 5.76 kW 


Before discussing the specialized techniques used to measure power in 
three-phase systems (Sec. 12-6), it will be to our advantage to consider first 
how a wattmeter is used in a single-phase circuit. 

Power measurement is most often accomplished at frequencies below 
a few hundred Hz through the use of a wattmeter which contains two 
separate coils. One of these coils is made of heavy wire, having a very 
low resistance, and is called the current coil; the second coil is composed 
of a much greater number of turns of fine wire, with relatively high 
resistance, and is termed the potential coil, or voltage coil. Additional 
resistance may also be inserted internally or externally in series with the 
potential coil. The torque applied to the moving system and the pointer 
is proportional to the instantaneous product of the currents flowing in the 
two coils. The mechanical inertia of the moving system, however, causes 
a deflection which is proportional to the average value of this torque. 

The wattmeter is used by connecting it into a network in such a way 
that the current flowing in the current coil is the current flowing into the 
network and the voltage across the potential coil is the voltage across the 
two terminals of the network. The current in the potential coil is thus 
the input voltage divided by the resistance of the potential coil. The 
wattmeter deflection is therefore proportional to the average power de- 
livered to the network. 

It is apparent that the wattmeter has four available terminals, and 
correct connections must be made to these terminals in order to obtain 
an upscale reading on the meter. To be specific, let us assume that we 
are measuring the power absorbed by a passive network. The current coil 


(+ +£V Potential 



I t 

10 n 

V rms \^ 

' ( 




v 2 = 

loo a° 

V rms 



Fig. 12-19 (a) A wattmeter connection that will ensure an upscale reading 
for the power absorbed by the passive network, (b) An example in which the 
wattmeter is installed to give an upscale indication of the power absorbed 
by the right source. 

is inserted in series with one of the two conductors connected to the load, 
and the potential coil is installed between the two conductors, usually on 
the "load side" of the current coil. The potential coil terminals are often 
indicated by arrows, as shown in Fig. 12- 19a. Each coil has two terminals, 
and the proper relationship between the sense of the current and voltage 
must be observed. One end of each coil is usually marked ( + ), and an 
upscale reading is obtained if a positive current is flowing into the ( + ) 
end of the current coil while the ( + ) terminal of the potential coil is 
positive with respect to the unmarked end. The wattmeter shown in the 
network of Fig. 12-19a therefore gives an upscale deflection when the 
network to the right is absorbing power. 

A reversal of either coil, but not both, will cause the meter to try to 
deflect downscale; a reversal of both coils will never affect the reading. 

As an example of the use of such a wattmeter in measuring average 
power, let us consider the circuit shown in Fig. 12-19£>. The connection 
of the wattmeter is such that an upscale reading corresponds to a positive 
absorbed power for the network to the right of the meter, that is, the right 
source. The power absorbed- by this source is given by 

P= |V 2 ||I|cos(angV 2 -angI) 

Using superposition or mesh analysis, the current is found, 

I = 11.18 /153.4° A rms 

and thus the absorbed power is 

P = (100)(11.18) cos (0° - 153.4°) = -1000 W 

The pointer therefore rests against the downscale stop. In practice, the 
potential coil may be reversed more quickly than may the current coil, 
and this reversal provides an upscale reading of 1000 W. 


337 Polypha*» Circuits 

Drill Problem 

12-10 In the circuit of Fig. 12-20, determine whether or not the potential coil 
must be reversed to obtain an upscale reading and find that reading for the ideal 
wattmeter: (a) A; (b) B; (c) C. 

Ans. reversed, 15 W; as is, 35 W; as is, 70 W 

Fig. 12-20 See Drill Prob. 12-10. 


At first glance, the measurement of the power drawn by a three-phase load 
seems to be a simple problem. We need place only one wattmeter in each 
of the three phases and add the results. For example, the proper connec- 
tions for a Y-connected load are shown in Fig. 12-21o. Each wattmeter 
has its current coil inserted in one phase of the load and its potential coil 
connected between the line side of that load and the neutral. In a similar 

Fig. 12-21 Three wattmeters are connected in such a way that each reads 
the power taken by one phase of a three-phase load, and the sum of the 
readings is the total power, (a) A Y-connected load, [b) A A-connected load. 
Neither the loads nor the source need be balanced. 

Fig. 12-22 A method of connecting three wattmeters to measure the total 
power taken by a three-phase load. Only the three terminals of the load are 

way, three wattmeters may be connected as shown in Fig. 12-21& to 
measure the total power taken by a A-connected load. The methods are 
theoretically correct, but they may be useless in practice because the 
neutral of the Y is usually not accessible and the phases of the A are not 
available. A three-phase rotating machine, for example, has only three 
accessible terminals, those we have been calling A, B, and C. 

It is obvious that we need a method for measuring the total power drawn 
by a three-phase load having only three accessible terminals; measurements 
may be made on the "line" side of these terminals, but not on the "load" 
side. Such a method is available, and it is capable of measuring the power 
taken by an unbalanced load from an unbalanced source. Let us connect 
three wattmeters in such a way that each has its current coil in one line 
and its voltage coil between that line and some common point x, as shown 
in Fig. 12-22. Although a system with a Y-connected load is illustrated, 
the arguments presented below are equally valid for a A-connected load. 
The point x may be some unspecified point in the three-phase system, or 
it may be merely a point in space at which the three potential coils have 
a common node. The average power indicated by wattmeter A must be 

1 r T 

P A = J J V A*'a. 


where T is the period of all the source voltages. The readings of the other 
two wattmeters are given by similar expressions, and the total average 
power drawn by the load is therefore 

1 r T 
P = P A + P B + F C~jJ ( v aJ*a + v bAb + v cJcc 



339 Polyphase Circuits 

Each of the three voltages in the above expression may be written in terms 
of a phase voltage and the voltage between point x and the neutral, 

v a* = v an + %x 

V B, = V BN + %* 

and, therefore, 

P ~ J J ( V AN'aA + VBNhB + «Wcc) * + jf » Wl (W + h B + >c< 



However, the entire three-phase load may be considered to be a supernode, 
and Kirchhoff's current law requires 

*oa + Hb + he = ° 


( C At/iaA + «W&B + VCN'cc) * 

Reference to the circuit diagram shows that this sum is indeed the sum 
of the average powers taken by each phase of the load, and the sum of 
the readings of the three wattmeters therefore represents the total average 
power drawn by the entire load. 

Let us illustrate this procedure by a numerical example before we 
discover that one of these three wattmeters is really superfluous. We shall 
assume a balanced source, 

V o6 = 100/01 V rms 
V* = 100 7-120° 
V ca = 100 / -240° 

or V„„ = -^/-30° 

V — -IPJ)-/_1V>° 

V CT = -^ /-270° 

and an unbalanced load, 

Z A = -;10 J2 
Z B = ,10 

340 Sinusoidal Analysis 

Let us assume ideal wattmeters, connected as illustrated in Fig. 12-22, with 
point x located on the neutral of the source n. The three line currents 
may be obtained by mesh analysis, 

I 100/0° -/10 I 

I 100/^1201 10 + , 10 1 =1 Arms 

aA I -;10 I 

I -;10 10 4-/10 I 

and by similar methods, 

I bB = 19.3/165° I cC = 10 /-90" 

The voltage between the neutrals is 

V„ ff = V„ 6 + y £N = \ b + I 6B (;10) = 157.8Z=9Q!. 
Thus, the average power indicated by each wattmeter may be calculated, 

F A = V phA COS ( an § \n ~ an g \a) 

= iPO, 19.3 cos (15° + 30°) = 788 W 

Vz ' 

P„ = -i5Ll9.3 cos (165° + 150°) = 788 W 

P r = i2Ll0cos(-90° +270°)= -577 W 
c V3 

or a total power of 999 W. Since an rms current of 10 A flows through 
the resistive load, the total power drawn by the load is 

P = 10 2 (10) = 1000 W 

and the three-wattmeter method checks within slide-rule accuracy. 

It is interesting to note that the reading of one of the wattmeters is 
negative. The discussion of the use of the wattmeter in the previous section 
indicates that an upscale reading on that meter can be obtained only after 
either the potential coil or the current coil is reversed. 

We have proved that point x, the common connection of the three 
potential coils, may be located any place we wish without affecting the 
algebraic sum of the three wattmeter readings. Let us now consider the 
effect of placing point x, this common connection of the three wattmeters, 
directly on one of the lines. If, for example, one end of each potential 
«oil is returned to E, then there is no voltage across the potential coil of 
wattmeter B and this meter must read zero. It may therefore be removed, 

34 1 Polyphase Circuits 

and the algebraic sum of the remaining two wattmeter readings is still the 
total power drawn by the load. When the location of * is selected in this 
way, we describe the method of power measurement as the two-wattmeter 
method. The sum of the readings indicates the total power, regardless of 
(1) load unbalance, (2) source unbalance, (3) differences in the two watt- 
meters, and (4) the waveform of the periodic source. The only assumption 
we have made is that wattmeter corrections are sufficiently small so that 
we can ignore them. In Fig. 12-22, for example, the current coil of each 
meter has passing through it the line current drawn by the load plus the 
current taken by the potential coil. Since the latter current is usually quite 
small, its effect may be estimated from a knowledge of the resistance of 
the potential coil and the voltage across it. These two quantities enable 
a close estimate to be made of the power dissipated in the potential coil. 
In the numerical example described above, let us now assume that two 
wattmeters are used, one with current coil in line A and potential coil 
between lines A and B, the other with current coil in line C and potential 
coil between C and B. The first meter reads 

F i = V AB ! aA cos (ang V AB - ang I„J 
= 1000(19.3) cos (15° -0°) 
= 1866 W 

and the second 

and, therefore, 

p 2 = Vcuhc cos (ang V CB - ang I cC ) 
= 100(10) cos (-90° - 60°) 
= -866 W 

P = P l + P 2 = 1866 - 866 = 1000 W 

This we know is the correct answer. 

In the case of a balanced load, the two-wattmeter method enables the 
PF angle to be determined, as well as the total power drawn by the load. 
Let us assume a load impedance with a phase angle 0; either a Y or A 
connection may be used and we shall assume the A connection shown in 
Fig. 12-23. The construction of a standard phasor diagram, such as that 
of Fig. 12-18, enables us to determine the proper phase angle between the 
several line voltages and line currents. We therefore determine the readings 

p i = I v ab\ 14* I cos (ang V^ - angl„j 
= V L I L cos (30° + 9) 

Fig. 12-23 Two wattmeters connected to read the total power drawn by 
a balanced three-phase load. 


h = I Veal \hc\ cos(angV CB - angI cC ) 

= V,, cos (30° - 6) 
The ratio of the two readings is 

p i cos (30° + 0) 

P 2 cos (30° - 6) 
If we expand the cosine terms, this equation is solved easily for tan 0, 


tan«= V^f— ^ 

P2 + P1 


Thus, equal wattmeter readings indicate a unity PF load, equal and opposite 
readings indicate a purely reactive load, a reading of P 2 which is (alge- 
braically) greater than P 1 indicates an inductive impedance, and a reading 
of P 2 which is less than P x signifies a capacitive load. How can we tell 
which wattmeter reads P x and which reads P 2 ? It is true that P 1 is in line 
A, and P 2 is in line C, and our positive phase-sequence system forces V aB 
to lag V cn . This is enough information to differentiate between the two 
wattmeters, but it is confusing to apply in practice. Even if we were unable 
to distinguish the two, we know the magnitude of the phase angle, but 
not its sign. This is often sufficient information; if the load is an induction 
motor, the angle must be positive and we do not need to make any tests 
to determine which reading is which. If no previous knowledge of the load 
is assumed, then there are several methods of resolving the ambiguity. 
Perhaps the simplest method is that which involves adding a high- 
impedance reactive load, say a three-phase capacitor, across the unknown 


343 Po'yphaie Circuit* 

load. The load must become more capacitive. Thus, if the magnitude of 
tan (or the magnitude of 6) decreases, then the load was inductive, whereas 
an increase in the magnitude of tan 6 signifies an original capacitive im- 

Let us suppose that one meter indicates 30 W while the other reads 
100 W. Since we are assuming a passive load, the sign of the larger reading 
must be positive, but we must determine the sign of the smaller reading 
by a careful inspection of the location of the coil terminals marked ( + ). 
Let us assume that we know that it actually represents a negative power. 
Thus, P 1 is either -30 or 100, and P 2 is either 100 or -30. The value 
of tan# is therefore either 3.22 or —3.22, and the power-factor angle is 
either 72.7° or —72.7°. We then place three capacitors across the load 
in a balanced arrangement and find that the reading which was — 30 W 
is now —27 W, while the 100- W reading has increased to 104 W. Since 
neither reading has changed appreciably, we decide that the capacitors 
have an impedance which is sufficiently high to produce only an incre- 
mental change, and we may calculate the new phase angle; it is either 
+ 71.3° or —71.3°. The load must now be more capacitive than it was 
previously, and the only conclusion that can be drawn is that the phase 
angle was originally 72.7°, whereas now it is 71.3°. 

Drill Problems 

12-1 1 Three ideal wattmeters are arranged as shown in Fig. 12-22. Let V ab = 
125/01 V rms, Z A = Z B = Z c = 24 - ;7 Q, point x be on point C, and the phase 
sequence be positive. Find: (a) P A ; (b) P B ; (c) P c . 

Ans. 0; 249; 351 W 

12-12 Identify the source and load sides of a three-phase three- wire transmission 
system by a, b, c and A, B, C, respectively, and assume positive phase sequence 
witn \i> — 125/01 V rms. One phase current in the balanced A-connected load 
is *ab — 8/ — 45° A rms. The current coil of an ideal wattmeter is inserted in 
line aA, ( + ) terminal toward a. Find the wattmeter reading if the ( + ) and ( — ) 
terminals of the potential coil are connected to: (a) A and B; (b) A and C; (c) 
B and C, all respectively. 

Ans. 448; 1225; 1673 W 

12-13 The two-wattmeter method is used to measure the total power taken by 
a balanced three-phase load, known to be passive. What is the PF of the load 
if: (a) one wattmeter reads 0; (b) the magnitude of one wattmeter reading is twice 
the magnitude of the other; (c) the magnitudes of the two wattmeter readings 
are equal? 

Ans. or 1.000; 0.189 or 0.866; 0.500 

344 Sinusoidal Analysis 


□ 1 Given a balanced six-phase system in which V on = 20/01, V^ = 20/ — ( 

, V M = 20/-300°, find: (a) V o6 ; (b) V de ; (c) V„ ; (d) V c 

D 2 A single-phase three-wire system operates with \ an = V nb = 120 /0 ° V rms. 
Lines aA and bB each have 0.1 SI of resistance while the neutral wire has 1.0 £2. 
(a) If Z AN = Z BN = 6/01 and Z^ = 8/Q1 fi, find I^. (fc) Find 1^ if Z BN is 
open-circuited, (c) Find 1^ if both Z BN and Z^ B are open-circuited. 

□ 3 A single-phase three-wire system is fed by V an = V nb = 100/0" V rms. The 
two outside line currents are l aA = 10 + /0 and I 6B = — 9 4- /l A rms. If load 
Z, AN is 25 + ;0 fl, find Z BW and 2, AB . Assume zero line resistance. 

D 4 A common 120/240-V rms single-phase three-wire household circuit has 
2.4-kVA loads across each 120-V line, one at unity PF and the other at 0.8 PF 
lagging. The 240-V load is 4.5 kW at 0.6 PF lagging. Find both line currents 
and the neutral current. 

□ 5 A balanced three-phase voltage source, V on = 200/0° V rms, positive phase 
sequence, is connected by four lossless conductors to an unbalanced load: 7, AS = 
20 + ;0, Z BN = 10 + ;10, Z ClV = 10 — /'10 S2. Find the three phasor line currents 
and the neutral current. 

□ 6 With reference to the circuit shown in Fig. 12-24, let V ab = 150/0° V rms 
and assume positive phase sequence. If Z p = 3 — ;4 Q, find the rms line current 
and the total power delivered to the load if: (a) R w = 0; (b) R w = 0.2 Q. 



z„ —U 

Fig. 12-24 See Probs. 6 and 8. 

D 7 A three-phase induction motor requires 6 kW at 0.8 PF lagging. Determine 
the values for a Y of capacitors that will produce net unity PF operation when 
placed in parallel with the motor on a balanced 250-V rms (line voltage) system 
for which / = 60 Hz. 

345 Polyphase Circuits 

□ 8 In the balanced three-phase circuit shown in Fig. 12-24, V an = 120 /0° V rms 
and the source provides 3600 VA at PF = 0.75 lagging. Assuming positive phase 
sequence with R w = 0.5 fl, find: (a) Z p ; (b) the transmission efficiency. 

□ 9 A balanced three-phase voltage source, V an = 200 /0° V rms, positive phase 
sequence, is connected to an unbalanced A load: X AB — 60 + /0, Z BC = 30 + /30, 
X CA = 30 — /30 fi. Find: (a) the three phasor line currents; (h) the power de- 
livered to each phase of the load; (c) the power provided by each phase of the 

n 10 In the circuit shown in Fig. 12-17, V an = 150 /0" V rms with positive phase 
sequence. If X p = 3 — ;4 fi, find the rms line current and the total power de- 
livered to the load. 

□ 1 1 Find the line current, the total power delivered to the load, and the total 
power loss in the lines for the circuit of Fig. 12-25 if V ab = 180/0°. V rms, 
Z p = 7.5 + ;3 U, R w = 0.5 Q, and positive phase sequence is assumed. 

Fig. 12-25 See Prob. 11. 

□ 12 A three-phase motor draws 9 kVA at a lagging PF of 0.8 from a balanced 
system with line voltages of 300 V rms at 60 Hz. Three capacitors of what size 
should be arranged as a parallel A-connected load to produce unity PF operation? 

□ 13 Given a balanced three-phase system for which V L = 450 V rms, two loads 
are present; one is Y-connected with an impedance of 20 — /10 U per phase, and 
the other is A-connected with 15 + ;30 Q per phase. Find the line current, the 
power delivered to each load, and the overall PF. 

□ 1 4 A A-connected source is slightly unbalanced. Each source phase is a practical 
voltage source with a resistance of 0.1 $2, but the three voltages are 100 /0° . 
101 / — 120° . and 99 /120° V rms. Find the source phase currents under no-load 
conditions and the total power loss in the source. 

D 15 Determine the impedance Z of the capacitor in the circuit shown in Fig. 
12-26 so that the wattmeter reading will be: (a) zero; (b) 18 W; (c) 3.6 W after 
potential coil reversal. 

Fig. 12-26 See Prob. 15. 

D 16 Determine the wattmeter reading in the circuit shown in Fig. 12-27. What 
is the physical interpretation of this reading? 

Kg. 12-27 See Prob. 16. 

□ 1 7 Show whether or not the two wattmeters in the circuit of Fig. 12-28 measure 
the total power taken by the general load consisting of Z 1( Z 2 , and Z 3 : (a) if 
Vj = V 2 ; (b) if Vj and V 2 have unequal magnitudes and phase angles. 







z 3 

/"" "X ^s~ 

v 2 Q 



z 2 



— »■ 

Fig. 12-28 See Probs. 17 ond 18. 

D 18 Refer to Fig. 12-28 and find the power indicated by each wattmeter if 
Z t = 4 + ;2, Z 2 = 4 - ;'2, Z 3 = 4 Q, V t = 120 /0° . and V 2 = 120 /120° V rms. 
What power is absorbed by each load? 

D 19 A balanced A-connected load is present on a 240-V rms (line voltage) three- 
phase system. The line current is 10 A rms. A wattmeter with its current coil 
in one line and its potential coil between the two remaining lines reads 1500 W. 
Describe the load impedance. 

D 20 Under what conditions will a single wattmeter read the total power taken 
by a balanced three-phase load in a three-wire system where the current coil 
is in one line and the potential coil is between the other two lines? 


Chapter Thirteen - 

Y3~1 ym 

We^i i&^gni the fourth major portion of ow study of Gi*£alt 

analyst, a dfsCB«d$M» of the concept of complex frequency. This, we'rfiijjfi', 
see. is a remarkably oniiying concept which irifl enable us to tie together 
all our prevjoosly de««loped analytical techniques into one neat package. 
ftestsSve^s^bitQSJkfysis, steady-state sinusoidal analysis, transient analysis, 
the fbpa^.- ft^Kwttft, <h© complete response, and the analysis of circuits 
i .excttfedjlfe'^paSBid^iai forcing functions and exponentially damped sinus- 
OidalftolBgfwftctteBS TriU all become special cases of the general tech- 
niques which are associated with the complex-frequency concept. 

352 Complex Frequency 

We shall introduce the concept of a complex frequency by considering 
an exponentially damped sinusoidal function, such as the voltage 

v(t) = V m e° t cos (cot + 8) (1) 

where a (sigma) is a real quantity and is usually negative. Although we 
refer to this function as being "damped," it is possible that the sinusoidal 
amplitude may increase if a is positive; the more practical case is that of 
the damped function. Our work with the natural response of the RLC 
circuit also indicates that a is the negative of the exponential damping 

We may first construct a constant voltage from (1) by letting both a 
and <o be zero, 

v(t) = V m cos0 = V (2) 

If we set only a equal to zero, then we obtain a general sinusoidal voltage 

v(t) = V m cos(o,t + 0) (3) 

And if to = 0, we have the exponential voltage 

v(t) = V m cos 6 e" ( = V e" (4) 

Thus, the damped sinusoid (1) includes as special cases the dc (2), sinusoidal 
(3), and exponential (4) forcing functions. 

Some additional insight into the significance of a can be obtained by 
comparing the exponential function (4) with the complex representation 
of a sinusoidal forcing function with a zero-degree phase angle, 

v(t) = V»< (5) 

It is apparent that the two functions, (4) and (5), have much in common. 
Their only difference is in the presence of a real and an imaginary expo- 
nent. The similarity between the two functions is emphasized by describing 
a as a "frequency." This choice of terminology will be discussed in detail 
in the following sections, but for now we need merely note that a is 
specifically termed the real part of the complex frequency. It should not 
be called the "real frequency," however, for this is a term which is more 
suitable for / (or, loosely, for io). We shall also refer to a as the neper 
frequency, the name arising from the dimensionless unit of the exponent 
of e. Thus, given e 2t , the dimensions of 2t are nepers (Np), and 2 is the 
neper frequency in nepers per second. The neper itself was named after 

353 Complex Frequency 

Napier and his napierian logarithm system; the spelling of his name is 
historically uncertain. 

A forcing function of damped sinusoidal or exponential form raises some 
questions with regard to its amplitude for large negative values of t when 
a < 0. That is, we have considered the forced response as that produced 
by a forcing function applied since t = — oo; its application at some finite 
time gives rise to a transient response in addition to the forced response. 
Since the infinite amplitude of the forcing function at r = — oo may make 
us somewhat uncomfortable, we might note that initial conditions can be 
established in any circuit so that the application of a specified forcing 
function at a specified instant of time produces no transient response. 
Examples of this will appear later. From a practical point of view, we 
know that, although it may be impossible to generate such forcing func- 
tions in the lab which are accurate for all time, we can produce approxi- 
mations that are satisfactory for circuits whose transient response does 
not last very long. 

The response of a network to this general forcing function (1) is found 
very simply by using a method almost identical with that used for the 
sinusoidal forcing function; we shall discuss the method in Sec. 13-4. When 
we are able to find the response to this damped sinusoid, we should realize 
that we shall also have found the response to a dc voltage, an exponential 
"voltage, and a sinusoidal voltage. Now let us see how we may consider 
a and <o as the real and imaginary parts of a complex frequency. 


Let us first provide ourselves with a purely mathematical definition of 
complex frequency and then gradually develop a physical interpretation 
in the next few sections. We shall say that any function which may be 
written in the form 

£(t) = Ke 8 ' (6) 

where K and s are complex constants (independent of time), is characterized 
by the complex frequency s. The complex frequency s is therefore simply 
the factor which multiplies t in this complex exponential representation. 
Until we are able to determine the complex frequency of a given function 
by inspection, it is necessary to write the function in the form of (6). 

We may apply this definition first to the more familiar forcing functions. 
For example, a constant voltage 

v(t) = V 

354 Complex Frequency 

may be written in the form 

v(t) = V e m 

The complex frequency of a dc voltage or current is thus zero; s = 0. The 
next simple case is the exponential function 

v{t) = V " 

which is already in the required form; the complex frequency of this voltage 
is therefore a; s = a + /0. Finally, let us consider a sinusoidal voltage, 
one which may provide a slight surprise. Given 

v(t) = V m cos (art + 8) 

it is necessary to find an equivalent expression in terms of the complex 
exponential. From our past experience, we therefore use tbi identity we 
derived from Euler's formula, 

cos (art + 8) = 1 / 2 (e*<* (+w + e -^ t+e >) 

and obtain 

or v(t) = (% vv»« + (y 2 v,^v*" 

We have the sum of two complex exponentials, and two complex fre- 
quencies are therefore present, one for each term. The complex frequency 
of the first term is s = s x = /<o and that of the second term is s = s 2 = — ;<o. 
These two values of s are conjugates, or s 2 = s*, and the two values of 
K are also conjugates. The entire first term and the entire second term 
are therefore conjugates, which we should expect inasmuch as their sum 
must be a real quantity. 

Now let us determine the complex frequency or frequencies associated 
with the exponentially damped sinusoidal function (1). We again use Euler's 
formula to obtain a complex exponential representation: 

v(t) = V m e ot cos (cot + 8) 

and thus 

v(t) = 1 / 2 V m e* 8 e ( " +, '' ,)< + %V m e-'V"- ,u " 

We therefore find once again that a conjugate complex pair of frequencies 
is required to describe the exponentially damped sinusoid, s t = a + ;co, and 
% = s* = a — jw. In general, neither a nor co is zero, and we see that the 

355 Complex Frequency 

exponentially varying sinusoidal waveform is the general case; the constant, 
sinusoidal, and exponential waveforms are special cases. 

As numerical illustrations, we should now recognize at sight the complex 
frequencies associated with these voltages: 

v(t) = 100 s = 

o(() = 5e~ 2t s = -2 + /0 

v(t) = 2 sin 500t 

v(t) = 4«r 3 'sin(6t + 10°) 

s 1 = /500 

s 2 = s* = -/500 

gj = -3 + ;6 

Sj = s* = -3 - ft 

The reverse type of example is also worth consideration. Given a 
complex frequency or a pair of conjugate complex frequencies, we must 
be able to identify the nature of the function with which they are associ- 
ated. The most special case, s = 0, defines a constant or dc function. With 
reference to the defining functional form (6), it is apparent that the constant 
K must be real if the function is to be real. 

Let us next consider real values of s. A positive real value, such as 
s = 5 + yO, identifies an exponentially increasing function Ke 5 ', where again 
K must be real if the function is to be a physical one. A negative real 
value for s, such as s = — 5 + /O, refers to an exponentially decreasing 
function Ke -5 '. 

A purely imaginary value of s, for example, /10, can never be associated 
with a real quantity; the functional form is Ke' 10t , which can also be 
written as K(cos 10* + / sin lOt), and obviously possesses both real and 
imaginary parts. Each part is sinusoidal in nature. In order to construct 
a real function, it is necessary to consider conjugate values of s, such as 
s 12 = ±/10, with which must be associated conjugate values of K. Loosely 
speaking, however, we may identify either of the complex frequencies 
Sj = ;10 or Sg = — ;10 with a sinusoidal voltage at the radian frequency 
of 10 rad/s. The presence of the conjugate complex frequency is under- 
stood. The amplitude and phase angle of the sinusoidal voltage will depend 
on the choice of K for each of the two frequencies. Thus, selecting % = /10 
and Kj = 6 — /8, where Sj = s* and Kg = K*, we obtain the real sinusoid 
20 cos (10* - 53.1°). 

In a similar manner, a general value for s, such as 3 — /5, can be 
associated with a real quantity only if it is accompanied by its conjugate 
3 + ;5. Speaking loosely again, we may think of either of these two 
conjugate frequencies as describing an exponentially increasing sinusoidal 
function e 3 ' cos 5t; the specific amplitude and phase angle will again depend 
on the specific values of the conjugate complex K's. 

356 Complex Frequency 

By now we should have achieved some appreciation of the physical 
nature of the complex frequency s; in general, it describes an exponentially 
varying sinusoid. The real part of s is associated with the exponential 
variation; if it is negative, the function decays; if positive, the function 
increases; and if it is zero, the sinusoidal amplitude is constant. The 
imaginary part of s describes the sinusoidal variation; it is specifically the 
radian frequency. It is customary to call the real part of s, a, and the 
imaginary part cc (not ;<o): 

s = a + ju (7) 

The radian frequency is sometimes referred to as the "real frequency," but 
this terminology can be very confusing when we find that we must then 
say that "the real frequency is the imaginary part of the complex fre- 
quency"! When we need to be specific, we shall call s the complex 
frequency, a the neper frequency, co the radian frequency, and / the cyclic 
frequency; when no confusion seems likely, it is permissible to use "fre- 
quency" to refer to any of these four quantities. The neper frequency is 
measured in nepers per second, radian frequency is measured in radians 
per second, and complex frequency s is measured in units which are 
variously termed complex nepers per second or complex radians per second. 

Drill Problems 

13-1 Determine all the complex frequencies associated with the voltage wave- 
form: (a) v(t) = -0.1(1 - 0.2e-°- 6 ' cos lOOf); (b) v(t) = 2 + 4e~ 0Mt - 6e-°- 4t ; (c) 
v(t) = 10e-°- 6( + 8 sin (lOOt + 15°). 

Am. -0.6, -1100, 1100; 0, -0.6 - 1100, -0.6 + 1100; 0, -0.6, -0.4 s" 1 

13-2 Find the complex frequencies associated with the natural response of a 
source-free parallel RLC circuit in which L = 10 / 9 H, C — 10 jwF, and R = : (a) 
oo; (b) 100 Q; (c) 62 %fi. 

Ans. -900, -100; -240 -1180, -240 + 1180; -j300, p00 s" 1 


The preceding discussion has shown us that the real and imaginary parts 
of the complex frequency describe, respectively, the exponential and 
sinusoidal variation of an exponentially varying sinusoid. It is apparent 
that the significance of a complex frequency is more general than is that 
of the everyday variety of frequency which describes the number of times 
some phenomenon repeats itself per unit time. Our ordinary concept of 
frequency, however, actually carries with it another connotation in addition 

35 7 Complex Frequency 

to "repetitions per second." It also tells us something about the rate of 
change of the function being considered. That is, high frequency means 
"rapidly varying." Let us see if we can relate this connotation of frequency 
to the complex frequency of a complex exponential function of time. We 
again take 

t(t) = Ke*> (8) 

After obtaining the time rate of change of f (t), 

4^ = sKe 8 ' 

we normalize by dividing by t(t), 


-^= s (9) 

This normalized rate of change is a constant, independent of time; it is 
identically equal to the complex frequency s. Thus, we may also interpret 
complex frequency as the normalized time rate of change of the complex 
exponential function (8). The use of this alternative definition of s on 
familiar functions which are not in the form of the complex exponential 
function (8) may lead to some curious results. Thus, although the complex 
frequency associated with the function e' 5 ' is s = ;5, the normalized rate 
of change associated with cos 5* must be (—5) tan5r. If we try to treat 
this result, which is a function of time, as a complex frequency, then we 
are led to a complex frequency which is a function of time. The correct 
answer to our problem is obtained only when we recognize that a conjugate 
pair of complex frequencies is required to characterize cos 5r; one complex 
frequency is insufficient. 

Drill Problem 

13-3 A network is composed of three different resistors and one capacitor in 
some configuration which is immaterial to this problem. No sources are present, 
but initial energy is present in the capacitor. The voltage waveform across the 
capacitor is displayed on an oscilloscope. At t — 30 ms, v c = 50 V, and it is 
decreasing at the rate of 1000 V/s. After finding the complex frequency which 
characterizes v c , write a suitable functional form for the voltage and determine 
the instant of time at which: (a) v c — 25 V; (b) the rate of change of v c is 
— 100 V/s; (c) the rate of change of v c is — 10 kV/s. 

Ans. -85; 64.7; 145 ms 

358 Complex Frequency 


We have devoted enough time to the definition and introductory inter- 
pretation of complex frequency; it is now time to put this concept to work 
and become familiar with it by seeing what it will do and how it is used. 
The general exponentially varying sinusoid, which we may represent 
as a voltage for the moment, 

v(t) = V m e°* cos (at + 6) (10) 

is expressible in terms of the complex frequency s by making use of Euler's 
identity as before: 

v(t) = Re(V m e"V ( "" +s) ) (11) 

or v(t) = Re (V m e"'e' < -"'- < ") (12) 

Either representation is suitable, and the two expressions should remind 
us that a pair of conjugate complex frequencies is associated with a sinusoid 
or an exponentially damped sinusoid. Equation (11) is more directly related 
to the given damped sinusoid, and we shall concern ourselves principally 
with it. Collecting factors, 

v(t) = Re (V m e> s e la+ >" H ) 
we now substitute s = a + /co, and obtain 

v(t) = Re (V m e> e e") (13) 

Before we apply a forcing function of this form to any circuit, we should 
note the resemblance of this last representation of the damped sinusoid 
to the corresponding representation of the undamped sinusoid, 

Re (V m e>V u( ) 

The only difference is that we now have s where we previously had /co. 
Instead of restricting ourselves to sinusoidal forcing functions and their 
angular frequencies, we have now extended our notation to include the 
damped sinusoidal forcing function at a complex frequency. It should be 
no surprise at all to see later in this section and the following one that 
we shall develop a frequency-domain description of the exponentially 
damped sinusoid in exactly the same way that we did for the sinusoid; we 
shall simply omit the Re notation and suppress e st . 

We are now ready to apply the exponentially damped sinusoid, as given 

359 Complex Frequency 

by (10), (11), (12), or (13), to an electrical network. The forced response, 
say a current in some branch of the network, is the desired response. Since 
the forced response has the form of the forcing function, its integral, and 
its derivatives, the response may be assumed to be 

i(t) = I m e ct cos (at + <J>) 
or i(t) = Re (I m e^e st ) 

where the complex frequency of the source and the response must be 

If we now recall that the real part of a complex forcing function 
produces the real part of the response, while the imaginary part of the 
complex forcing function causes the imaginary part of the response, then 
we are again led to the application of a complex forcing function to our 
network. We shall obtain a complex response whose real part is the desired 
real response. Actually, we shall work with the Re notation omitted, but 
we should realize that it may be reinserted at any time and that it must 
be reinserted whenever we desire the time-domain response. Thus, given 
the real forcing function 

v(t) = Re (V m e> s e at ) 

we apply the complex forcing function V m e> e e Bt ; the resultant complex 
response I m e'*e 8 ' must have as its real part the desired time-domain re- 

*(*) = Be (/„,«*•«") 

The solution of our circuit-analysis problem must consist of the determi- 
nation of the unknown response amplitude I m and phase angle <j>. 

Before we actually carry out the details of an analysis problem and 
see how exactly the procedure follows that which was used in the sinusoidal 
analysis, it is worthwhile outlining the steps of the basic method. We must 
first characterize the circuit with a set of loop or nodal integrodifferential 
equations. The given forcing functions, in complex form, and the assumed 
responses, also in complex form, are then substituted into the equations 
and the indicated integrations and differentiations performed. Each term 
in every equation will then contain the same factor e at . We shall therefore 
divide throughout by this factor, or "suppress e at ," understanding that it 
must be reinserted if a time-domain description of any response function 
is desired. Now that the Re symbol and the e at factor have disappeared, 
we have converted all the voltages and currents from the time domain to 
the frequency domain. The integrodifferential equations have become 
algebraic equations, and their solution is obtained just as easily as they were 


— v*A — onnr> — 

28 1 H 

»«>( + ) ^F=fe 

Fig. 13-1 A series RLC circuit to which a damped sinusoidal forcing func- 
tion is applied. A frequency-domain solution for i[t) is desired. 

in the sinusoidal steady state. Let us illustrate the basic method by a 
numerical example. 

We shall apply the forcing function 

v(t) = 60e"' cos (2f + 10°) 

to the series RLC circuit shown in Fig. 13-1, and we desire the forced 

i(t) = l m er' cos (2t + <j>) 

We first express the forcing function in Re notation, 

v(t) = 60e-' cos (2t + 10°) 
= Re (60e-V <2(+10O) ) 
= Re (6(V 10 V- 1+ > 2)f ) 
or v(t) = Re (Ve 8( ) 


V = 60Z1Q1 and s = - 1 + ;2 

After dropping Re, we are left with the complex forcing function 


In a similar manner, we represent the unknown response by the complex 


Since we have not as yet extended the impedance concept to the 
exponentially damped sinusoid and complex frequency, our next step must 


36 1 Complex Frequency 

be the integrodifferential equation for our circuit. From Kirchhoff's 
voltage law we obtain 

v{t) = Ri + L f t + lf idt 
= 2t + jf- + 2 fi dt 

and we substitute the given complex forcing function and the assumed 
complex response into this equation, 

60 /10° e s ' = 2Ie 8 ' + sle" + — Ie" 

The common factor e" is next suppressed: 

60 /10° = 21 + si + ^-1 

60 /10" 

2 + s + 2/s 

Before we evaluate this complex current, it is worth examining the form 
of this equation. The left side of the equation is a current, the numerator 
of the right side is a voltage, and the denominator must therefore have 
the dimensions of ohms; it is apparent that we shall soon interpret it as 
an impedance. Moreover, we might make some pretty astute guesses as 
to the impedance of each of the three passive elements at a complex 
frequency s. The impedance of the 2-S2 resistor is simply 2 0; the imped- 
ance of the 1-H inductor is Is or sL; and the impedance of the 0.5-F 
capacitor is 2/s or 1/sC. These statements will be proved in the following 

Going back to our numerical example, we now let s — — 1 + ;2 in the 
last equation and solve for the complex current I: 


2 + (-l + /2) + 2/(-l + /2) 
After manipulating the complex numbers for a few minutes, we find 

I = 44.8 / -53.4° 
Thus, l m is 44.8 A and <> is —53.4°. The desired forced response is thus 

iit) = 44.8e-' cos (2t - 53.4°) 

362 Complex Frequency 

Now we must show that the impedance concept may be extended to 
complex frequencies. Except for the presence of complex numbers, the 
actual solution of the circuit equations will then be no different than the 
procedure used for purely resistive circuits. 

Drill Problems 

13-4 Express each of the following currents in the frequency domain: (a) 
4e- 20 < cos (1000* + 60°) mA; (b) 4 sin (800* + 60°) mA; (c) -4e" 5 ' sin (1000* - 
60°) mA. 

Am. 4 / -30° ; 4 /30° : 4 /60° mA 

13-5 If V = 64 /80° V, find u(0.001) if s = : (a) -800 + /600; (b) -;600; (c) 
-800 - /600. 

Ans. -11.9; 20.1; 44.8 V 

13-5 Z(s) AND Y(s) 

In order to apply Kirchhoff 's laws directly to the complex forcing functions 
and complex responses, it is necessary to know the constant of propor- 
tionality between the complex voltage across an element and the complex 
current through it. This proportionality constant is the impedance or 
admittance of the element; it is easily determined for the resistor, inductor, 
and capacitor. 

Let us consider the inductor carefully and then merely present the 
results for the other elements. Suppose that a voltage source 

o(i) = V m e"" cos (ut + 6) 

is applied to an inductor L; the current response must have the form 

i(t) = l m e at cos (ut + <j>) 

The passive sign convention is employed, as indicated in Fig. 13-2o, the 
time-domain circuit. If we represent the voltage as 

v(t) = Re (V n e' s e B ') - Re (Ve<") 

and the current as 

i(t) = Re (l m e'*e at ) = Re (Ie 8< ) 

Ht) = l m e" cos (o)J + <t>) 

o(f) = V-e^cos (0)< + 9) 




Fig. 13-2 (a) The time-domain inductor voltage and current are related by 
V ~ L di/dt. (b) The (complex) frequency-domain inductor voltage and 
current are related by V = sLI. 

then the substitution of these expressions into the defining equation of an 

v(t) = L 


leads to 

Re (Ve 81 ) = Re (sLIe" 

We now drop Re, thus considering the complex response to a complex 
forcing function, and suppress the superfluous factor e 8 ': 

V = sLI 

The ratio of the complex voltage to the complex current is once again the 
impedance. Since it depends in general upon the complex frequency s, 
this functional dependence is sometimes indicated by writing 

Z(S) = -jr = SL 

In a similar manner, the admittance of an inductor L is 



We shall still call V and I phasors. These complex quantities have an 
amplitude and phase angle which, along with a specific complex-frequency 
value, enable us to characterize the exponentially varying sinusoidal wave- 
form completely. The phasor is still a frequency-domain description, but 
its application is not limited to the realm of radian frequencies. The 
frequency-domain equivalent of Fig. 13-2a is shown in Fig. \3-2b; phasor 
currents, phasor voltages, and impedances or admittances are now used. 


Fig. 13-3 The frequency-domain equivalent of the series RLC circuit shown 
in Fig. 13-1. 

The impedances of a resistor R and a capacitor C at a complex fre- 
quency s are obtained by a similar sequence of steps. Without going 
through the details, the results for a resistor are 

and for a capacitor 

Z(s) = R Y(s) = G = 1 

Z(s) = -~ *(«) = sC 

If we now reconsider the series RLC example of Fig. 13-1 in the 
frequency domain, the source voltage 

v(t) = me-* cos (2t + 10°) 

is transformed to the phasor voltage 

V = 60 /10° 

a phasor current I is assumed, and the impedance of each element at the 
complex frequency s = — 1 + ;2 is determined and placed on a fre- 
quency-domain diagram, Fig. 13-3. The unknown current is now easily 
obtained by dividing the phasor voltage by the sum of the three impedances: 

60 /10° 

2 + (-1 +/2) + 2/(-l +/2) 

Thus, the previous result is obtained, but much more easily and rapidly. 

It is hardly necessary to say that all the techniques which we have used 
in the past to simplify frequency-domain analysis, such as superposition, 
source transformations, duality, Thevenin's theorem, and Norton's theorem, 
are still valid and useful. For example, the Thevenin equivalent of the 
network shown in Fig. 13-4a is obtained as follows: 

The complex frequency is 

s = -5 + /10 

■ 20 + ;io a 

100e- 5 'cos 10< 

V (*) 


s = -5 + 

/so v Ars 
+ ;io W 


Fig. 13-4 (a) A given two-terminal network, [b] The frequency-domair 
Thevenin equivalent. 


The frequency-domain source voltage is 

v s = loo/o: 

The inductor impedance is 

Zt(s) = 4(-5 + /10) = -20 + /40 
The resistor impedance is 

Z»(«) = 20 
The Thevenin impedance is the parallel equivalent of Z t and Z R : 

20(-20 + /40) 
Z '> = 20-20 + /40 - 2 ° + ' 10 

The open-circuit voltage is 

\r = 100/0° 


" 20 - 20 + /40 

= -;50 

The frequency-domain Thevenin equivalent network is thus as shown 
in Fig. 13-4b. The return to the time domain is taken after some desired 
response has been determined in the frequency domain. If another 4-H 
inductor is placed across the open circuit, for example, the fre- 
quency-domain current is 



20 + f'10 - 20 + ;40 

corresponding to the time-domain current 

i(t) = —e~ 5t cos lOt 

366 Complex Frequency 

Drill Problems 

13-6 Find the input impedance Z(s) for the network shown in Fig. 13-5 as 
presented at terminal pair: (a) a-b; (h) c-d; (c) a-c. 

3(s + 4) 2(s 2 + 3) s(4s + 3) 

"*' 2(s 2 + 4s + 3) ; s 2 + 4s + 3 ; 2(s 2 + 4s + 3) 

o d 
Fig. 13-5 See Drill Probs. 13-6 to 13-8. 

13-7 For part (c) of Drill Prob. 6 above, find Z(s) at s = : (a) 0; (b) oo; (c) 
-2 + ;1. 

Ans. — 6 + \4; 2; 2 fi 

1 3-8 For the network shown in Fig. 13-5, find v ci (t) if a current source connected 
at terminals a-b delivers at node a a current of: (a) 8e~ 2 ' A; (b) 8 cos 3t A; 
(c) 8e" 2( cos 3t A. 

Ans. 24e- 2 ',- 2.6S cos (3f - 26.6°); 4.33e~ 2t cos (3t - 56.3°) V 


We have already considered circuit response as a function of the radian 
frequency w, representing such quantities as impedance, admittance, spe- 
cific voltages or currents, voltage and current gain, and transfer impedances 
and admittances as functions of w, determining their poles and zeros, and 
sketching the response. Before we discuss the more general problem of 
frequency response as a function of the complex frequency s in the next 
section, let us devote a little time to the simpler problem of frequency 
response as a function of o. 

As a simple example we may select the series RL circuit excited by 
the frequency-domain voltage source V m /0° . The current is obtained as 
a function of s by dividing the source voltage by the input impedance, 

I = 

R + sL 

We now set a> = 0, s = a + /0, thus restricting ourselves to time-domain 

367 Complex Frequency 

sources of the form 
and thus 

V m e° 

I = 

R + oL 

L a + R/L 


Transforming to the time domain, 

The necessary information about the response, however, is all contained 
in the frequency-domain description (14). As the neper frequency o varies, 
a qualitative description of the response is easily provided. When a is a 
large negative number, corresponding to a rapidly decreasing exponential 
function, the current response (14) is negative and relatively small in 
amplitude; it is, of course, also a rapidly decreasing (in magnitude) expo- 
nential function. As a increases, becoming a smaller negative number, the 
magnitude of the negative response increases. When a is exactly equal to 
— R/L, a pole of the response, the current amplitude is infinite. 

As a continues to increase, the next noteworthy point occurs when 
a = 0. Since v s = V m , we are now faced with the dc case, and the response 
is obviously V„JR, which agrees with the response indicated by (14). 
Positive values of a must all provide positive amplitude responses, the larger 
amplitudes arising when a is smaller. Finally, an infinite value of a provides 
a zero-amplitude response, and thus establishes a zero. The only critical 
frequencies are the pole at a — —R/L and the zero at a = ±oo. 

This information may be presented quite easily by plotting \I\, the 
current magnitude, as a function of a, as shown in Fig. 13-6. In preparation 
for the more general response information with changing s in the next 
section, we show the magnitude of I versus a; the phase (not shown) is, 
of course, either or 180°. 

Let us now turn our attention to the two critical frequencies of this 
response. The only finite critical frequency is the pole at a — —R/L. It 
is worthwhile to determine why an infinite response is obtained when the 
circuit is excited at this frequency by the voltage 

v = V m e- Rt/L (16) 

The forcing function (16) has a familiar form; it has all the characteristics 

Fig. 13-6 A plot of the magnitude of I versus neper frequency a for a 
series RL circuit excited by an exponential voltage source, V^'. The only 
pole is located at a = — R/L; the zero occurs at a = ±co. 

of the natural response. As a matter of fact, if we reduce the amplitude 
of this forcing function to zero, thus "exciting" the circuit by a short circuit, 
then the current 

i = I n e- m/L 


would flow if an initial current / were assumed. Although this is a natural 
response, it is informative to interpret the result as a forced response; we 
find that a zero-amplitude forcing function then produces a non-zero- 
amplitude response. Since the circuit is linear, a non-zero-amplitude 
forcing function must produce an infinite response. 

We shall find that this result is quite general; when any circuit is excited 
at a frequency which is a pole of the response, then an infinite response 
must result; the frequencies of the poles and zeros are directly related to 
the natural response of the circuit. This relationship will be seen to arise 
in several examples discussed in this section, but we shall not disucuss it 
thoroughly until the following section. 

As a second example, let us consider the circuit drawn in Fig. 13-7o. 
The exponential current source 

i = I m e°< 

is applied to a series RC circuit. The voltage across the source is given 


V=IZ(«) = l.(H + i) 

, a + l/RC 

V=I m R- 




Fig. 1 3-7 (a) A series RC circuit excited by an exponential current source, 
(fo) The magnitude of the voltage response possesses a pole at a = and a 
zero at a = — 1/RC. 

This last form of the voltage response, written as a constant times the ratio 
of factors having the form (a + a J, is obviously well suited for the quick 
determination of the poles and zeros of the response. The voltage response 
indicates a pole at a = and a zero at o = - 1/RC; infinite frequency 
is not a critical frequency. The response magnitude |V| is plotted as a 
function of frequency in Fig. 13-7fo. The reason for the pole at zero 
frequency may again be explained on physical grounds; if I m = 0, the 
current source is effectively an open circuit and the response is the constant 
initial capacitor voltage; a nonzero J m ' must therefore produce an infinite 
voltage response. In other words, if a constant current has been applied 
to the network forever, then the capacitor must have charged to an infinite 
voltage. All poles are of course a consequence of the ideal models we are 
assuming to represent the physical devices; a real capacitor would only 
permit the voltage to increase to some large value before its dielectric broke 

A more complicated response curve is obtained for the circuit shown 
in Fig. 13-8fl. The current is easily found: 


6 + a + 5/a 

1= 100 

(a + l)(a + 5) 


The response curve is most easily obtained by first indicating the locations 
of all poles and zeros on the a axis, and placing vertical asymptotes at 
the poles. When this is done, we find that a relative minimum of the 
response must exist between the two poles, and a relative maximum must 
be present at some frequency greater than zero. By differentiation, the 
locations of this minimum and maximum may be determined as a = — V§ 
and o = V5, respectively. The value of the response at the minimum turns 

» <r 

M (b) 

Fig. 13-8 {a) A series RLC circuit is driven by an exponential forcing func- 
tion, [b) The resultant current-magnitude response curve shows zeros at 
a = and a =±oo, and poles at a = —5 and —1 Np/s. 

out to be 65.5 and that of the maximum, 9.55. To emphasize the rela- 
tionship between the time domain and frequency domain once again, the 
response at a — —3 is found from (19) to be 75 A; hence, excitation of 
the network by the forcing function v(t) = 100e" 3( produces the forced 
current response i(t) — 75e -3t . 

The two poles may again be identified as the natural resonant frequen- 
cies of the circuit. That is, ,the transient response of an RLC circuit has 
the form 

*i„ = A^' + A 2 e°- 

where s x and Sg are given by 

w ~ 2L~V\2L/ LC 

- 1 and — 5 

Thus, a zero-amplitude forcing function at either of these two frequencies, 
a — —1 or a = —5, is associated with a finite amplitude response, the 
natural response of the circuit; a non-zero-amplitude forcing function 
provides an infinite response or a pole. 

Drill Problems 

1 3-9 If v s represents an exponential forcing function in the circuit shown in 
Fig. 13-9a, find all critical frequencies in the frequency-domain response ^ and 
sketch |/j| versus a. 

Am. -4; -1.23; -0.271; Np/s 


0.3 a* 

40 a 


* \ <<r) 


Fig. 13-9 (a) See Drill Prob. 13-9. [b] See Drill Prob. 13-10. 

13-10 For the circuit shown in Fig. 13-9&, find all critical frequencies of V c (a) 
and sketch |V C | versus a. 

Ans. -100; -33.3; 0; ±oo Np/s 

13-11 A two-terminal network is driven by the source 0Ae at A. The voltage 
across the source is the response, and it has a pole at a = — 2 and a zero at 
o = - 1 Np/s. When a = 0, V = 4 V. Write an expression for V(a) and evaluate 

it at a = : (a) -1.6; (b) -6; (c) - oo Np/s. 

An*. -i2; 8; 10 V 

13-12 The impedance Z(a) may be viewed as a response by considering it as 
the voltage produced by a current of unit amplitude. Assume that Z(o) has a 
zero at a = -5 and a pole at o = —1; the impedance is 12 fl at infinite fre- 
quency. Find: (a) Z(0); (b) Z(-3); (c) Z(-6). 

Ans. - i2; 2.4; 60 S2 


Now that we have considered the response of a circuit as u varies (with 
a = 0) and as a varies (with co = 0), we are prepared to develop a more 
general graphical presentation by graphing quantities as functions of s; that 
is, we wish to show the response simultaneously as functions of both a and 


Such a graphical portrayal of the response as a function of the complex 
frequency s is a useful, enlightening technique in the analysis of circuits, 
as well as in the design or synthesis of circuits. After we have developed 
the concept of the complex-frequency plane, or s plane, we shall see how 
quickly the behavior of a circuit can be approximated from a graphical 
representation of its critical frequencies in this s plane. The converse 
procedure is also very useful; if we are given a desired response curve (the 
frequency response of a filter, for example), it will be possible to decide 
upon the necessary location of its poles and zeros in the s plane and then 
to synthesize the filter. This synthesis problem is a subject for detailed study 
in subsequent courses and is not one which we shall do more than briefly 

372 Complex Frequency 

examine here. The s plane is also the basic tool with which the possible 
presence of undesired oscillations is investigated in feedback amplifiers and 
automatic control systems. 

Let us develop a method of obtaining circuit response as a function 
of s by extending the methods we have been using to find the response 
as a function of either a or to. To review these methods, let us obtain the 
driving-point impedance of a network composed of a 3-fi resistor in series 
with a 4-H inductor. As a function of s, we have 

Z(s) = 3 + 4s 

If we wish to obtain a graphical interpretation of the impedance variation 
with a, we let s = a + /0, 

Z(o) = 3 + 4o 

and recognize a zero at a = — % and a pole at infinity. These critical 
frequencies are marked on a a axis, and after identifying the value of Z(o) 
at some convenient noncritical frequency [perhaps Z(0) = 3], it is easy to 
sketch |Z(a)| versus a. 

In order to plot the response as a function of the radian frequency u, 
we let s = + ;w, 

Z(p) = 3 + ;4u 

and then obtain both the magnitude and phase angle of Z(/co) as functions 
of w: 

|Z(/to)| = V9 + 16co 2 
angZ(/<o) = tan" 1 -^ 

The magnitude function shows a single pole at infinity and a minimum 
at to = 0; it can be readily sketched as a curve of |Z(/to)| versus to. The 
phase angle is an inverse tangent function, zero at to = and ±90° at 
to = ±oo; it is also easily presented as a plot of ang Z(/to) versus o>. 

In graphing the response Z(/to) as a function of u, two two-dimensional 
plots are required, magnitude and phase angle as functions of w. When 
exponential excitation is assumed, we could present all the information on 
a single two-dimensional graph by permitting both positive and negative 
values of Z(a) versus a. However, we chose to plot the magnitude of Z(a) 
in order that our sketches would compare more closely with those depicting 
the magnitude of Z(/to). The phase angle (±180° only) of Z(a) was largely 
ignored. The important point to note is that there is only one independent 

373 Complax Frequency 

variable, a in the case of exponential excitation and <o in the sinusoidal 
case. Now let us consider what alternatives are available to us if we wish 
to plot a response as a function of s. 

The complex frequency s requires two parameters, a and <o, for its 
complete specification. The response is also a complex function, and we 
must therefore consider sketching both the magnitude and phase angle as 
functions of s. Either of these quantities, for example, the magnitude, is 
a function of the two parameters a and <o, and we can only plot it in two 
dimensions as a family of curves, such as magnitude versus u>, with a as 
parameter. Conversely, we could also show the magnitude versus a, with 
to as the parameter. Such a family of curves represents a tremendous 
amount of work, however, and this is what we are trying to avoid; it is 
also questionable whether we could ever draw any useful conclusions from 
the family of curves even after they were obtained. 

A better method of representing the magnitude of some complex 
response graphically involves using a t/We-dimensional model. Although 
such a model is difficult to draw on a two-dimensional sheet of paper, we 
shall find that the model is not difficult to visualize; most of the drawing 
will be done mentally, where few supplies are needed and construction, 
correction, and erasures are quickly accomplished. Let us think of a a axis 
and a /to axis, perpendicular to each other, laid out on a horizontal surface 
such as the floor. The floor now represents a complex-frequency plane, or 
s plane, as sketched in Fig. 13-10. To each point in this plane there 
corresponds exactly one value of s, and to each value of s we may associate 
a single point in this complex plane. 

Since we are already quite familiar with the type of time-domain 
function associated with a particular value of the complex frequency s, 
it is now possible to associate the functional form of a forcing function 
or response with the various regions in the s plane. The origin, for example, 
must represent a dc quantity. Points lying on the a axis must represent 
exponential functions, decaying for a < 0, increasing for a > 0. Pure 
sinusoids are associated with points on the positive or negative ju axis. 
The right half of the s plane, usually referred to simply as the RHP, contains 
points describing frequencies with positive real parts and thus corresponds 

fig. 13-10 The complex-frequency plane, or s plane. 

s plane 

Vv- .W 5 W 1 

Vv- VV 2 W 1 

Fig. 13-1 1 The nature of the time-domain function is sketched in the region 
of the complex-frequency plane to which it corresponds. 

to time-domain quantities which are exponentially increasing sinusoids, 
except on the a axis. Correspondingly, points in the left half of the s plane 
(LHP) describe the frequencies of exponentially decreasing sinusoids, again 
with the exception of the negative a axis. Figure 13-11 summarizes the 
relationship between the time domain and the various regions of the s plane. 

Let us now return to our search for an appropriate method of repre- 
senting a response graphically as a function of the complex frequency s. 
The magnitude of the response may be represented by constructing, say, 
a plaster model whose height above the floor at every point corresponds 
to the magnitude of the response at that value of s. In other words, we 
have added a third axis, perpendicular to both the a axis and the /'to axis 
and passing through the origin; this axis is labeled |Z|, |Y|, IVyVJ, or with 
whatever symbol is appropriate. The response magnitude is determined 
for every value of s, and the resultant plot is a surface lying above (or 
just touching) the s plane. 

Let us try out these preliminary ideas by seeing what such a plaster 



Fig. 13-12 (a) A cutaway view of a plaster model whose top surface 
represents (Y(S)J for the series combination of a 1-H inductor and a 3-fi 
resistor, (fo] |Y(s)| as a function of u. (c) |Y(s)| as a function of a. 

model might look like. As an example, we may consider the admittance 
of the series combination of a 1-H inductor and a 3-S2 resistor, 

¥(.) = 

s + 3 

In terms of both a and co we have, as the magnitude, 

|Y(s)j = 

V(o + 3) 2 4- , 

When s = — 3 + jO, the response magnitude is infinite; and when s is 
infinite, the magnitude of Y(s) is zero. Thus our model must be infinitely 
high over the point ( — 3 + yO), and it must be zero height at all points 
infinitely far away from the origin. A cutaway view of such a model is 
shown in Fig. 13-12a. 

Once the model is constructed, it is simple to visualize the variation 
of [Y| as a function of co (with a — 0) by cutting the model with a perpen- 
dicular plane containing the /co axis. The model shown in Fig. 13-12a 
happens to be cut along this plane, and the desired plot of |Y| versus w 
can be seen; the curve is also drawn in Fig. 13-12fo. In a similar manner, 
a vertical plane containing the a axis enables us to obtain |Y| versus a (with 
co = 0), shown in Fig. 13-12c. 

How might we obtain some qualitative response information without 
doing all this work? After all, most of us have neither the time nor the 


376 Complex Frequency 

inclination to be good plasterers, and some more practical method is 
needed. Let us visualize the s plane once again as the floor and then imagine 
a larger rubber sheet laid on it. We now fix our attention on all the poles 
and zeros of the response. At each zero, the response is zero, the height 
of the sheet must be zero, and we therefore tack the sheet to the floor. 
At the value of s corresponding to each pole, we may prop up the sheet 
with a thin vertical rod. Zeros and poles at infinity must be treated by 
using a large radius clamping ring or a high circular fence, respectively. 
If we have used an infinitely large, weightless, perfectly elastic sheet, tacked 
down with vanishingly small tacks, and propped up with infinitely long, 
zero-diameter rods, then the rubber sheet assumes a height which is exactly 
proportional to the magnitude of the response. Less accurate rubber-sheet 
models may actually be constructed in the laboratory, but their main 
advantage lies in the ease by which their construction may be visualized 
from a knowledge of the pole-zero locations of the response. 

These comments may be illustrated by considering the configuration 
of the poles and zeros, sometimes called a pole-zero constellation, which 
locates all the critical frequencies of some frequency-domain quantity, say 
the impedance Z(s). Such a pole-zero constellation is shown in Fig. 13-13a. 
If we visualize a rubber-sheet model, tacked down at s = — 2 + /0 and 
propped up at s = — 1 + ;5 and — 1 — /5, we should see a terrain whose 
distinguishing features are two mountains and one conical crater or depres- 
sion. The portion of the model for the upper left half of the s plane is 
shown in Fig. 13-13fo. 

Let us now build up the expression for Z(s) which leads to this pole-zero 
configuration. The zero requires a factor of (s + 2) in the numerator, and 
the two poles require the factors (s + 1 — ;5) and (s + 1 + /5) in the 
denominator. Except for a multiplying constant k, we now know the form 
of Z(s): 

Fig. 13-13 (a) The pole-zero constellation of some impedance Z(s). (b) A 
portion of the rubber-sheet model of the magnitude of Z{s). 

-1 +|5 




s plane 


377 Complex Frequency 

Z(s) = k 
Z(s) = k 

s + 2 

[s + 1 - /5)(s + 1 + /5) 
s + 2 

s 2 + 2s + 26 


Let us select k by assuming a single additional fact about Z(s); let Z(0) = 1. 
By direct substitution in (20), we find that k is 13, and therefore 

Z(s) = 13 

s + 2 

s 2 + 2s + 26 


The plots |Z(a)| versus a and |Z(/co)| versus <o may be obtained exactly 
from (21), but the general form of the function is apparent from the 
pole-zero configuration and the rubber-sheet analogy. Portions of these 
two curves appear at the sides of the model shown in Fig. 13-13fc. 

Thus far, we have been using the s plane and the rubber-sheet model 
to obtain qualitative information about the variation of the magnitude of 
the frequency-domain function with frequency. It is possible, however, to 
get quantitative information concerning the variation of both the magnitude 
and phase angle. The method provides us with a powerful new tool. 

Consider the representation of a complex frequency in polar form, as 
suggested by an arrow drawn from the origin of the s plane to the complex 
frequency under consideration. The length of the arrow is the magnitude 
of the frequency, and the angle that the arrow makes with the positive 
direction of the a axis is the angle of the complex frequency. The frequency 
s x = -3 + /4 = 5 /126.9° is indicated in Fig. 13- 14a. 

Fig. 13-14 (a) The complex frequency Sj = — 3 + /4 is indicated by 
drawing an arrow from the origin to s v [b) The frequency s = ;7 is also 
represented vectorially. (c) The difference s — Sj is represented by the vector 
drawn from Sj to s. 

> a 




s > 


S- Sj / 

1 1 




378 Complex Frequency 

It is also necessary to represent the difference between two values of 
s as an arrow or vector on the complex plane. Let us select a value of 
s that corresponds to a sinusoid s = f7 and indicate it also as a vector, as 
shown in Fig. 13-14£>. The difference s — s x is seen to be the vector drawn 
from the last-named point Sj to the first-named point s; the vector s — s t 
is drawn in Fig. 13- 14c. Note that s a + (s — Sj) = s. Numerically, s — s 1 = 
ft — (-3 + ;4) = 3 + ;3 = 4.24 /45° , and this value agrees with the 
graphical difference. 

Let us see how this graphical interpretation of the difference (s — s x ) 
enables us to determine frequency response. Consider the admittance 

Y(s) = s + 2 

Fig. 13-15 {a) The vector representing the admittance Y(s) = s + 2 is 
shown for s = /w. [b) Sketches of |Y(/to)j and ang Y(/to} as they might be 
obtained from the performance of the vector as s moves up or down the /to 
axis from the origin. 

379 Complex Frequency 

This expression may be interpreted as the difference between some fre- 
quency of interest s and a zero location. Thus, the zero is present at 
Sg = — 2 + /0, and the factor s + 2, which may be written as s — s 2 , is 
represented by the vector drawn from the zero location ^ to the frequency 
s at which the response is desired. If the sinusoidal response is desired, 
s must lie on the /to axis, as illustrated in Fig. 13-15a. The magnitude of 
s + 2 may now be visualized as to varies from zero to infinity. When s 
is zero, the vector has a magnitude of 2 and an angle of 0°. Thus Y(0) = 2. 
As co increases, the magnitude increases, slowly at first, and then almost 
linearly with to; the phase angle increases almost linearly at first, and then 
gradually appro aches 90 ° as o> becomes infinite. At to = 7, Y(/7) has a 
magnitude of \/2 2 + 7 2 and has a phase angle of tan -1 (3.5). The magni- 
tude and phase of Y(s) are sketched as functions of to in Fig. 13-156. 

Let us now construct a more realistic example by considering a fre- 
quency-domain function given by the quotient of two factors, 

We again select a value of s which corresponds to sinusoidal excitation 
and draw the vectors s + 2 and s + 3, the first from the zero to the chosen 
point on the /to axis and the second from the pole to the chosen point. 
The two vectors are sketched in Fig. 13-16a. The quotient of these two 
vectors has a magnitude equal to the quotient of the magnitudes and a 
phase angle equal to the difference of the numerator and denominator phase 
angles. An investigation of the variation of the magnitude of V(s) versus 
to is made by allowing s to move from the origin up the joi axis and 
considering the ratio of the distance from the zero to s = /to and the distance 
from the pole to the same point on the /to axis. The ratio evidently is % 
at to = and approaches unity as ui becomes infinite. A consideration of 
the difference of the two phase angles shows that ang \(joi) is 0° at to =0, 
increases at first as ic increases since the angle of the vector s + 2 is greater 
than that of s + 3, and then decreases with a further increase in co, finally 
approaching 0° at infinite frequency, where both vectors possess 90° 
angles. These results are sketched in Fig. 13- 16b. Although no quantitative 
markings are present on these sketches, it is important to note that they 
may be obtained easily. For example, the complex response at s = /4 must 
be given by the ratio 

V4 + 16 /tan" 1 (%) 

V(/4) = ' ^L 

V9+ 16 /tan-'(y 3 ) 

V(/4) = y^T /tan- 1 2 - tan-' (%) 

= 0.894 /10.3° 

» u 


Fig. 13-16 (a) Vectors are drawn from the two critical frequencies of the 
voltage response V(s) = (s + 2)/(s + 3). (b) Sketches of the magnitude and 
phase angle of Vjf'co) as obtained from the quotient of the two vectors shown 

In designing networks to produce some desired response, the behavior 
of the vectors drawn from each critical frequency to a general point on 
the ;'<o axis is an important aid. For example, if it were necessary to increase 
the hump in the phase response of Fig. 13-16£>, we can see that we must 
provide a greater difference in the angles of the two vectors. This may 
be achieved in Fig. 13-16a either by moving the zero closer to the origin 
or by locating the pole farther from the origin, or both. 

The ideas we have been discussing to help in the graphical determi- 
nation of the magnitude and angular variation of some frequency-domain 
function with frequency will be needed in the following chapter when we 
investigate the frequency performance of highly selective filters, or resonant 
circuits. These concepts are fundamental in obtaining a quick, clear un- 
derstanding of the behavior of electrical networks and other engineering 
systems. The procedure is briefly summarized as follows: 

Draw the pole-zero constellation of the frequency- domain function 
under consideration in the s plane, and locate a test point corre- 
sponding to the frequency at which the function is to be evaluated. 


381 Complex Frequency 

2 Draw an arrow from each pole and zero to the test point. 

3 Determine the length of each pole arrow and zero arrow and the 
value of each pole-arrow angle and zero-arrow angle. 

4 Divide the product of the zero-arrow lengths by the product of the 
pole-arrow lengths. This quotient is the magnitude of the fre- 
quency-domain function for the assumed frequency of the test point 
[within a multiplying constant, since F(s) and kF(s) have the same 
pole-zero constellations]. 

5 Subtract the sum of the pole-arrow angles from the sum of the 
zero-arrow angles. The resultant difference is the angle of the 
frequency-domain function, evaluated at the frequency of the test 
point. The angle does not depend upon the value of the real 
multiplying constant k. 

Drill Problems 

13-13 An impedance consists of a 2.5-mH inductor in series with the parallel 
combination of a 5-fi resistor and a 50-fiF capacitor. Find all the critical frequen- 
cies of Z(s) and draw the pole-zero configuration. 

Ans. -2 - j2; -2 + \2; -4; oo krad/s 

13-14 For the pole-zero constellations shown in Fig. 13-17, assume that they 
represent a voltage ratio Vj/Vj, and that the value of the ratio at infinite 
frequency is 20. Express the ratios as ratios of polynomials in s. 

20s 2 -80 20s + 200 20s 3 + 1600s 2 + 40,000s 


s 2 + 4 ' s + 20 ' s 3 + 20s 2 -)- 2500s + 50,000 


-20 -10 


-40 -20 



fig. 13-17 See Drill Prob. 13-14. 


1 20 







13-15 In a certain network, the output current I 2 produced by an input voltage 
Vj is found to have poles at —3 — /4 and — 3 + ;4, and zeros at — 1 + /0 and 

382 Complex Frequency 

— 4 + jO. A plaster model of the response function ^/Vj has a height of 8 cm 
at the origin. What is its height at s = : (a) -2; (b) -2 - /2; (c) 2 + ;2? 

Ans. 5.88; 23.2; 27.1 cm 

13-16 A pole-zero configuration shows zeros at — 1 ± /4 and poles at — 1 ±/2. 
By sketching this constellation and visualizing the pertinent vectors, estimate the 
positive radian frequency at which the response: (a) magnitude is a minimum; 
(b) magnitude is a maximum; (c) phase angle is a negative maximum (= —90°). 
Ans. 1.5, 3, 4 (approx.); 1.43, 3.02, 4.47 (exact) rad/s 


There is a tremendous amount of information contained in the pole-zero 
plot of some response in the s plane. We shall find out how the complete 
current response, natural plus forced, produced by an arbitrary voltage 
forcing function can be quickly written from the pole-zero configuration 
of the impedance offered to the voltage source and from the initial condi- 
tions; the method is similarly effective for the dual problem, the complete 
voltage response produced by a current source. 

Let us introduce the method by considering the simplest example, a 
series RL circuit as shown in Fig. 13-18. A general voltage source v(t) causes 
the current i(t) to flow after closure of the switch at t = 0. The complete 
response i(t) is composed of a natural response and a forced response: 

i(t) = i n (t) + i f (t) (22) 

We may find the forced response by working in the frequency domain, 
assuming, of course, that v(t) has a functional form which we can transform 
to the frequency domain; if v(t) — t 2 , we must proceed as best we can from 
the basic differential equation for the circuit. Here we have 

W = E 7TWI (231 

and i f (t) is obtained by replacing s, L, and R by their values, reinserting 
e"*, and taking the real part. The answer may even be obtained as a function 
of a general <o, a, R, and L if desired. 

Now let us consider the natural response. Of course, we know that 
the form will be a decaying exponential with the time constant L/R, but 
we may pretend that we are finding it for the first time. The natural 
response or source-free response is, by definition, of a form independent 

Fig. 13-18 An example which illustrates the determination of the complete 
response through a knowledge of the critical frequencies of the impedance 
faced by the source. 

of the forcing function; the forcing function contributes, along with the 
other initial conditions, only to the magnitude of the natural response. To 
find the proper form, replace all independent sources by their internal 
impedances; here, v(t) is replaced by a short circuit. Now let us try to 
obtain this natural response as a limiting case of the forced response; we 
return to the frequency-domain expression (23) and obediently set V(s) = 0. 
On the surface, it appears that I(s) must also be zero, but this is not 
necessarily true; the denominator may be zero. In other words, if we apply 
no voltage at the frequency s = —R/L, some current at this frequency 
may flow. It is of course necessary that there be some energy stored initially 
in the circuit for this to occur. 

Let us inspect this new idea from a slightly different vantage point. 
The forced response to the given voltage source is 

If we happen to apply a voltage at the exact frequency of one of the zeros 
of Z(s), then an infinite current will flow. This is true even though only 
1 juV is applied. We then conclude that a finite current at this frequency 
may flow even though no voltage is applied. Since the circuit is now 
source-free, that current is of the form of the source-free or natural re- 

Returning to our series RL circuit, we see by (23) that infinite current 
results when the operating frequency is s = — R/L + p. A finite current 
at this frequency thus represents the natural response 

I(s) = A at s = - ^ + /0 

Transforming this natural response to the time domain, 

i„(t) = Re {Ae- Rt ' L ) 
or •„(*) = Ae~ R " L 







Fig. 13-19 The zeros of Z(s) determine the form of the natural response 
of the current which would be present in a short circuit across the input 

To complete this example, the total response is then 

i(t) = Ae~ Rt/L + i f (t) 

and A may be determined once the initial conditions are specified for this 

Now let us generalize these results. Figure 13-19 shows a general 
two-terminal network that contains no independent sources. The input 
impedance may be written in a form which displays all the critical fre- 

Z( S ) 

_ k (* ~ s t )(s - %) • • 
(s - s 2 )(s - s 4 ) • • 


It is customary to designate the zeros of an impedance or the poles of an 
admittance by odd-numbered subscripts; impedance poles and admittance 
zeros receive even-numbered subscripts. Hence, the zeros of Z(s) occur 
at s = Sj, s = s 3 , etc., and if a voltage is applied to the input terminals 
at any of these frequencies, infinite current will flow. Thus, a finite current 
at each of these frequencies must be a possible functional form for the 
natural response. Therefore, we think of a zero-volt source (which is just 
a short circuit) applied to the input terminals; the natural response which 
occurs when the input terminals are short-circuited must thus have the form 

i n (t) = Aje"' + A 3 e*< + • • • 

where the A's must be evaluated in terms of the initial conditions (including 
the initial value of any voltage source applied at the input terminals). 
Let us now consider the dual of this problem. Again we may refer 
to the network shown in Fig. 13-19, but let us suppose for the moment 
that a current source is applied at the input terminals. The input voltage 
response is then 

V(s) = I( S )Z(s) 


385 Complex Frequency 

If we happen to apply a current at the frequency of one of the poles of 
Z(s), an infinite-amplitude input voltage results; it follows then that if we 
apply a zero-amplitude current (an open circuit) at this frequency, a finite 
response may be present at the same frequency. This is a source-free 
response, and it is identifiable as the natural response. Hence, if we assume 
the input impedance is expressed in the form of (24), then the functional 
form of the natural voltage response across the open-circuited input termi- 
nals must be 

v n (t) = A 2 e 8 *' + A 4 e 9 << + • • ■ 

The open-circuit natural voltage response is composed of a sum of terms 
at the frequencies of the poles of the input impedance or, stated slightly 
differently, at the frequencies of the zeros of the input admittance. The 
short-circuit natural current response is composed of a sum of terms at 
the frequencies of the zeros of the input impedance or the poles of the 
input admittance. 

Let us now try out these techniques on two examples. The first circuit 
is shown in Fig. 13-20, and it is identical with that of Fig. 5-13, a network 
whose natural response was found earlier with a great deal of difficulty. 
Let us again find the form of i x and i 2 . Considering i x first, we must find 
a suitable location for the short circuit through which this current flows; 
let us use the points marked x and x'. The input impedance viewed from 
these terminals when they are open-circuited is 

Z(s) = 2 S + l + 3^ 
or Z( S ) = 2 —^ 

Thus, i x must be of the form 

i,(f) = Aje" 2 ' + A 3 e~' /6 

Fig. 13-20 The circuit shown in Fig. 5-13 is redrawn here. The natural 
responses lj and tg are desired. 

386 Com P'«x Frequency 

The solution is completed by using the given initial conditions (ij and t 2 
are both 11 A at t = 0) to establish the values of A x and A 3 . Although 
we have been able to obtain the form of the solution much more rapidly 
than we did before, we cannot shorten the procedure for evaluating the 
unknown constants; any saving in effort here must come later with a study 
of the Laplace transform. For practice, let us complete the solution for 
i v Since i 1 (0) is given as 11, then 

11 = A 1 + A 3 

The necessary additional equation is obtained by differentiating j a : 

di 1 

— — 2A X — / 6 A 3 

But Zdijdt is the voltage across the 2-H inductor, and Kirchhoff 's voltage 
law shows that this must be the sum of the initial voltages across the two 
resistors. Thus 


11 + 22 

— — 2Ai — /s^-3 

Thus, Aj = 3 and A 3 — 8, and the desired solution is 

i t (t) = 3«r 2 < + 8e~ (/6 

The solution for i 2 obtained in Chap. 5 may be checked by inspecting the 
impedance obtained when the right-hand mesh is broken. 

As our last example we shall find the complete response v(t) of the circuit 
shown in Fig. 13-21. The switch is closed prior to t = 0, and thus all 
currents and voltages to the right of the switch are initially zero. At t — 
the switch is opened, and the voltage across the switch is to be found. 
This response is composed of both a forced and a natural response, 

v(t) = v n (t) + v f (t) 

Fig. 13-21 A circuit whose complete response is to be found through 
investigation of its critical frequencies. 

12 n 
-W. — i 

Ht) = JL t - Olj 

cos«a(>) > ' 

J'« 1' 

u) < 3 a 


SH |6H 

387 Complex Frequency 

Each may be found through a knowledge of the pole-zero configuration 
of the input impedance or admittance of the portion of the network to 
the right of the switch. Remembering that an inactive current source is 
an open circuit, and that the switch is also an open circuit for t > 0, the 
natural response v n {t) is thus composed of a sum of terms, each term 
corresponding to a pole of the input impedance or a zero of the input 
admittance. We have for Y(s) 

Y u = i + i + 6TTT2 

or, after combining and factoring, 

The form of the natural response may now be written 

v n (t) = A 2 e'< + A 4 e- 3 ' 

In order to find the forced response, the frequency-domain current 
source I(s) = 1 at s = — 1 + /2 may be divided by the input admittance, 
evaluated at s = — 1 + ;2, 

VW = ^= 1 

¥(•) Y(-l + /2) 
(-l + /2)(l + /2) 

m + / 2 ) 

and thus 

V(s) = 1.875 V2 745° 

Transforming to the time domain, we have 

v f (i) = 1.875 V2V' cos (2t + 45°) 
The complete response is therefore 

u(t) = A 2 e-' + A 4 e" 3 ' + 1.875 V2>' cos (2f + 45°) 

Since the current through both inductors is initially zero, the initial source 
current of 1 A must flow through the 3-fi resistor. Thus 

„(0) = 3 = A 2 + A 4 + i^^ (26) 


388 Complex Frequency 

Again it is necessary to differentiate and then to obtain an initial condition 
for dv/dt. We first find 

= 1.875 ^(--^--U-A.-M, 

dv _ 

dt\ t=0 - * - v - -p- ^r, - - 2 - —4 

or %\ = - 5 - 625 - A 2 - 3A 4 (27) 

The initial value of this rate of change is obtained by analyzing the circuit. 
However, those rates of change which are most easily found are the 
derivatives of the inductor currents, for v — L di/dt, and the initial values 
of the inductor voltages should not be difficult to find. We therefore express 
the response v(t) in terms of the resistor current, 

v(t) = 3i R 

and then apply Kirchhoff 's current law, 

v(t) = 3»— 3i w - 3t L2 

Now we may take the derivative, 

dv _ 3 di_ _ 3 di^ _ 3 di L2 
dt dt dt dt 

Differentiation of the source function and evaluation at t = provide a 
value of —3 V/s for the first term; the second term is numerically % °f 
the initial voltage across the 2-H inductor, or —4.5 V/s; and the last term 
is -1.5 V/s. Thus, 

dv I = _9 
dt I (=0 

and we may now use (26) and (27) to determine the unknown amplitudes 

A 2 = A 4 = 1.125 

The complete response is therefore 

v(t) = 1.125e- 3i + 1.875 V2e-' cos (2t + 45°) 

In spite of the detailed process which we must pursue to evaluate the 
amplitude coefficients of the natural response, except in those cases where 

389 Complex Frequency 

the initial values of the desired response and its derivatives are obvious, 
we should not lose sight of the ease and rapidity with which the form of 
the natural response can be obtained. 

Drill Problems 

13-17 Find the frequency components present in the natural response i(t) of 

Fig. 13-22 when a charged 3-fiF capacitor is suddenly connected to terminals: 

(a) a~b; (b) b-c; (c) a-c. 

Am. -698, -79.6; -500, -111; -50 kNp/s 

1 AlF sfc 


Fig. 13-22 See Drill Prob. 13-17. 

13-18 The circuit shown in Fig. 13-23 contains stored energy at t = 0. Find 
the complex frequencies present in the response o(t) for t > 0. 

Arts. -1; -2; -3 Np/s 


Fig. 13-23 See Drill Prob. 13-18 and Prob. 13-22. 

13-19 Find all the complex frequencies present in the complete voltage response 
v(t) in the circuit of Fig. 13-24 for t > if v,(t) = 20(cos lOOOrt)u(i) V. 

Ans. ±jl000w; ±jl000; ±j2000 s~ x 

Fig. 13-24 See Drill Prob. 13-19. 



jH 1»*F 

sk jH3«(!) 

100 kO 

500 kn l j^ 

Fig. 13-25 See Drill Prob. 13-20. 

1 3-20 For the circuit shown in Fig. 13-25, find the complete response: (a) v(t); 
(h) i 2 (t); (C) i^t). 

Ans. 0.1(e~ 2 ' - e- 5t )u(t) mA; (0.4e~ 2t + 0.2e- 5t )u(t) mA; 
(60 - 100e~ 2t + 40e~ 5t )u(t) V 


D 1 If V(s) = 2s + 10/s, find v(t) for s = : (a) - 2; (b) ;4; (c) - 2 + /4; (d) - 2 - ;4. 

□ 2 If i(t) is represented by the sum Ajg 81 ' + Aje" 2 ', find A x , A 2 , s 1; and s 2 if i{t) = : 
(a) 6e~ 2t cos 3f; (b) 6 e - 2 ' sin (3f + 30°); (c) 6 cos 3t; (d) 6e" 2( . 

D 3 The current, i s = 0.36"' cos at A, is present in the admittance Y(s) = 0.01 + 
0.6/s. Find the resultant voltage v(t) if: (a) a = - 10, u = 0; (b) a = 0, <o = 30; 
(c) a = - 10, u = 30. 

D 4 Let i s = 2e- 3000 ' cos (4000t + 21°) mA in the circuit shown in Fig. 13-26. 
Find: (a) v^t); (b) v 2 (t). 

Fig. 13-26 See Prob. 4. 

□ 5 The voltage 80e~ 3 ' sin 4f V is present across the series combination of a 20-fi 
resistor and a 4-H inductor. Assume steady-state conditions and determine the 
total energy delivered to the combination after t = 0. 

□ 6 A capacitor C is in parallel with the series combination of a 10-fi resistor 
and an inductor L. Determine C and L so that the input impedance of the parallel 
combination possesses a: (a) zero at s = — 100; (b) pole at — 100 + /20 s* 1 . 


391 Complex Frequency 

□ 7 Given an RLC series circuit, determine the element values so that the input 
admittance has poles at -20 ± ;140 s" 1 and |Y(;100)| =0.18. 

□ 8 Sketch Z(or) and |Z(<j)| versus o for the network shown in Fig. 13-27 if the 
unknown element is: (a) a short circuit; (b) an open circuit; (c) a 6-fi resistor; 
(d) a 2-H inductor; (e) a 10 4 -jiF capacitor. 

o 'VSS^- 

12 Q. 

Rg. 1 3-27 See Probs. 8 and 9. 

□ 9 Make the sketches requested in Prob. 8 if the unknown element in the circuit 
of Fig. 13-27 is a dependent voltage source, positive reference on top, labeled 
2i in , where i in is the current to the right in the 6-H inductor. 

□ 10 For each of the three networks shown in Fig. 13-28, determine all the critical 
frequencies of the input impedance and indicate their locations on the s plane. 

10 Q 10 fi 10 fi 

|SH §2H SJ2H 9iH |SH §2H 

See Prob. 10. 

□ 1 1 The series branches R^ and R 2 -C 2 are connected in parallel. Find all 
critical frequencies of the admittance of the parallel combination if R 1 = 
R 2 = 50 a, C 2 = 1 tiF, and L x = : (a) 1.6 mH; (b) 2.5 mH; (c) 5 mH. 

□ 1 2 A 10-12 resistor is in series with the parallel combination of a 20-fi resistor 
and a 5-H inductor. Make a pole-zero plot of Z(s) on Jthe s plane and prepare 
a qualitative sketch of |Z| versus a and |Z| versus u. 

□ 13 Make an s-plane plot of the poles and zeros of the transfer admittance, 
Y = Ij/%, for the circuit shown in Fig. 13-29. Using this plot, sketch |Y| versus 
<o; indicate values at w = and <o = oo. 

□ 1 4 Determine the voltage gain V (s)/V 1 (s) for the transistor-amplifier equivalent 
circuit shown in Fig. 13-30. Locate all critical frequencies of the ratio on the 
s plane and sketch the gain magnitude as a function of <o. 



R9. 13-29 See Prob. 13. 

Fig. 13-30 See Prob. 14. 

□ 1 5 The circuit of Fig. 13-31 shows an equivalent circuit for a transformer (Chap. 
15). Determine the poles and zeros and sketch the magnitude versus o> curve 
for the ratio: (a) I 2 /I i; (b) V^. 

Fig. 13-31 See Prob. 15. 

□ 16 An admittance Y(s) has only one pole and one zero. When s = — 1, —3, 
and ±00, Y(s) = 3, 1, and 5 0, respectively. Find an expression for Y(s) and locate 
the critical frequencies in the s plane. 

□ 17 The voltage ratio V 2 /\ f° r the circuit shown in Fig. 13-32 has a pole at 
-100 + ;700. If R = 500 fi, find L and C. 

Fig. 13-32 See Prob. 17. 




V 2 


393 Complex Frequency 

□ 1 8 The critical frequencies of a certain impedance are zeros at s = — 1 ± ;10 
and poles at s = and oo. Let |Z| be 2 U at s = — 1 + ;0. (a) Determine the 
expression for Z(s). (b) Sketch |Z(/<o)| versus w. (c) By considering the form of 
Z(s), find the simplest circuit that will provide this impedance. 

□ 19 A battery V^,, an open switch that closes at t = 0, and an impedance 
Z(s) = 2(s 4- 2)/(s + 4) are in series, (a) Determine the appropriate form for the 
current in the circuit after t = 0. (b) Evaluate the unknown amplitudes by making 
use of the information that i(0 + ) = 6 A and di/dt = 12 A/s at t = 0+. (c) After 
being closed for a long time, now assume that the switch is opened at t = 0. 
Determine v(t), the voltage across the impedance, if c(0 + ) = — 12 V. 

□ 20 With reference to the circuit shown in Fig. 13-33, let Z(s) = 2(s + 6)/(s + 2). 
(a) Determine the form for e(t), t > 0, except for unknown amplitudes, (b) If 
u(0 + ) = 1 V and u'(0 + ) = 4 V/s, determine v(t) for t > 0. (c) Assume the 
switch has been open for a very long time and let it close at t = 0. Assume 

«(0+) = 1 A and find i(t), t > 0. 


,.(t) ,-.-V J 





Fig. 13-33 See Prob. 20. 

□ 21 An admittance Y(s) has a zero at s = —6 and a pole at s = —2. Furthermore, 
Y(oo) = 0.2 H. (a) Find Y(s). (b) A 12-V battery and a switch are placed in series 
with Y(s). The switch is closed at t = 0. Find i(t) if i(0+) = 2.4 A. 

□ 22 Find v(t) for t > in the circuit of Fig. 13-23 if the given initial conditions 
are: (a) c(0) = 1, t/(0) = -2, e"(0) = 6; (b) c(0) = 2, i(0) = 3/20, t'(0) = 1/60. 

Chapter Fourteen 
Frequency Response 


Frequency response is a subject that has come up for consideration several 
times before. In Chap. 10 we discussed plots of admittance, impedance, 
current, and voltage as functions of <o. and the pole-zero concept was 
introduced as an aid in constructing and interpreting response curves. 
Response as a function of the neper frequency a was discussed from the 
same standpoint in the last chapter. At that time, we also broadened our 
concept of frequency and introduced the complex frequency s and the s 
plane. We found that a plot of the critical frequencies of a response on 
the complex-frequency plane enabled us to tie together the forced response 

395 Frequency Response 

and the natural response; the critical frequencies themselves presented us 
almost directly with the form of the natural response, and the visualization 
of a three-dimensional rubber-sheet model or the performance of vectors 
drawn from each critical frequency to some test frequency gave us valuable 
information concerning the variation of the forced response with frequency. 

In this chapter, we shall concentrate again on the forced response, and 
we shall particularly consider its variation with the radian frequency w. 

Why should we be so interested in the response to sinusoidal forcing 
functions when we so seldom encounter them in practice as such? The 
electric power industry is an exception, for the sinusoidal waveform appears 
throughout, although it is sometimes necessary to consider other frequencies 
introduced by the nonlinearity of some devices. But in most other electrical 
systems, the forcing functions and responses are not sinusoidal. In any 
system in which information is to be transmitted, the sinusoid by itself is 
almost valueless; it contains no information because its future values are 
exactly predictable from its past values. Moreover, once one period has 
been completed, any periodic nonsinusoidal waveform also contains no 
additional information. 

Sinusoidal analysis, however, provides us with the response of a network 
as a function of to, and the later work in Chaps. 18 and 19 will develop 
methods of determining network response to aperiodic signals (which can 
have a high information content) from the known sinusoidal frequency 

The frequency response of a network provides useful information in 
its own right, however. Let us suppose that a certain forcing function is 
found to contain sinusoidal components having frequencies within the range 
of 10 to 100 Hz. Now let us imagine this forcing function being applied 
to a network which has the property that all sinusoidal voltages with 
frequencies from zero to 200 Hz applied at the input terminals appear 
doubled in magnitude at the output terminals, with no change in phase 
angle. The output function is therefore an undistorted facsimile of the input 
function, but with twice the amplitude. If, however, the network has a 
frequency response such that the magnitudes of input sinusoids between 
10 and 50 Hz are multiplied by a different factor than are those between 
50 and 100 Hz, then the output would in general be distorted; it would 
no longer be a magnified version of the input. This distorted output might 
be desirable in some cases and undesirable in others. That is, the network 
frequency response might be chosen deliberately to reject some frequency 
components of the forcing function, or to emphasize others. 

The importance of frequency response is not limited to electrical 
systems, however; an understanding of electrical frequency response is 
certainly helpful in analyzing the frequency response of, say, a mechanical 
system. Suppose that we consider the launching of a space vehicle. The 
booster will subject the entire vehicle to extreme nonsinusoidal vibration, 

396 Com P lex Frequency 

the mechanical forcing function, with frequency components from a few 
Hz up to perhaps 50 Hz. The structural members of every stage will be 
deflected or distorted, the mechanical response, by an amount which 
depends on the sinusoidal components of the vibrational forces and on the 
frequency response of the structure. From this information, a prediction 
as to whether or not the space vehicle can survive the rigors of the launch 
operation can be made. If the mechanical response at some vibration 
frequency is found to be excessive, then that component of the booster 
vibration must be reduced, a redesign of the supporting structure must be 
undertaken, or some vibration dampers (filters) must be provided. 

This example should not make us think that it is undesirable to have 
the network response at some particular frequency be much larger than 
the response at all other frequencies. Such behavior is characteristic of 
tuned circuits or resonant circuits, as we shall see in this chapter. In 
discussing resonance we shall be able to apply all the methods we have 
discussed in presenting frequency response. 


In this section we shall begin the study of a very important phenomenon 
which may occur in circuits containing both inductors and capacitors. The 
phenomenon is called resonance, and it may be loosely described as the 
condition existing in any physical system when a fixed-amplitude sinusoidal 
forcing function produces a response of maximum amplitude. However, 
we often speak of resonance as occurring even when the forcing function 
is not sinusoidal. The resonant system may be electrical, mechanical, 
hydraulic, acoustic, or some other kind, but we shall restrict our attention 
to electrical systems. We shall define resonance more exactly below. 

Resonance is a familiar phenomenon. By jumping up and down on the 
bumper of an automobile, for example, the vehicle can be put into rather 
large oscillatory motion if the jumping is done at the proper frequency 
(about one jump per second), and if the shock absorbers are somewhat 
decrepit. However, if the jumping frequency is increased or decreased, 
the vibrational response of the automobile will be considerably less than 
it was before. A further illustration is furnished in the case of an opera 
singer who is able to shatter crystal goblets by means of a well-formed 
note at the proper frequency. In each of these examples, we are thinking 
of frequency as being adjusted until resonance occurs; it is also possible 
to adjust the size, shape, and material of the mechanical object being 
vibrated, but this may not be so easily accomplished physically. 

The condition of resonance may or may not be desirable, depending 
upon the purpose which the physical system is to serve. In the automotive 


Fig. 14-1 The parallel combination of a resistor, an inductor, and a capacitor, 
often referred to as a parallel resonant circuit. 

example above, a large amplitude of vibration may help to separate locked 
bumpers, but it would be somewhat disagreeable at 60 mi/h. 

Let us now define resonance more carefully. In a two-terminal electrical 
network containing at least one inductor and one capacitor, resonance is 
the condition which exists when the input impedance of the network is 
purely resistive. Thus, a network is said to be in resonance (or resonant) 
when the voltage and current at the network input terminals are in phase. 
We shall also find that a maximum-amplitude response is produced in the 
network when it is in the resonant condition or almost in the resonant 

We shall apply the definition of resonance to the parallel RLC network 
shown in Fig. 14-1. In many practical situations, this circuit is a very good 
approximation to the circuit we might build in the laboratory by connecting 
a physical inductor in parallel with a physical capacitor, where this parallel 
combination is driven by an energy source having a very high output 
impedance. The admittance offered to the ideal current source is 



and thus resonance occurs when 

«C - -T- = 

The resonant condition may be achieved by adjusting L, C, or to; we shall 
devote our attention to the case for which co is the variable. Hence, the 
resonant frequency <o is 



/« = • 


The pole-zero configuration of the admittance function can also be used 


398 Complex Frequency 

to considerable advantage here. Given Y(s), 

, s2 + s/RC + 1/LC 

Y(s) = C 


we may display the zeros of Y(s) by factoring the numerator, 

Y/s) = c ( s + » - i u d)( s + « + i^d) 

where a and to d represent the same quantities that they did when we 
discussed the natural response of the parallel RLC circuit in Sec. 7-2. That 
is, a is the exponential damping coefficient, 

and u d is the natural resonant frequency (not the resonant frequency <o ), 

u d = V« 2 - « 2 

The pole-zero constellation shown in Fig. 14-2a follows directly from the 
factored form. 

In view of the relationship among a, o> d , and co , it is apparent that 

Fig. 14-2 (a) The pole-zero constellation of the input admittance of a parallel 
resonant circuit is shown on the s plane; u 2 = a 2 + a d 2 . (b) The pole-zero 
constellation of the input impedance. 


" \ 


s plane 




s plane 




Fig. 14-3 The magnitude of the voltage response of a parallel resonant circuit 
is shown as a function of frequency. 

the distance from the origin of the s plane to one of the admittance zeros 
is numerically equal to <o . Given the pole-zero configuration, the resonant 
frequency may therefore be obtained by purely graphical methods. We 
merely swing an arc, using the origin of the s plane as a center, through 
one of the zeros. The intersection of this arc and the positive ju axis locates 
the point s = jo> . It is evident that to is slightly greater than the natural 
resonant frequency co d , but their ratio approaches unity as the ratio of oi d 
to a increases. 

Next let us examine the magnitude of the response, the voltage V(s) 
indicated in Fig. 14-1, as the frequency of the forcing function is varied. 
If we assume a constant-amplitude sinusoidal current source, the voltage 
response is proportional to the input impedance. This response can there- 
fore be obtained from the pole-zero plot of the impedance Z(s), shown in 
Fig. 14-2b. The response obviously starts at zero, reaches a maximum value 
in the vicinity of the natural resonant frequency, and then drops again to 
zero as <o becomes infinite. The frequency response is sketched in Fig. 14-3. 
The maximum value of the response is indicated as R times the amplitude 
of the source current, implying that the maximum value of the circuit 
impedance is simply R; moreover, the response maximum is shown to occur 
exactly at the resonant frequency to . The two frequencies <0j and <o 2 , which 
we shall see later will give us a measure of the width of the response curve, 
are also identified. Let us first show that the maximum impedance is R 
and that this maximum impedance occurs at resonance. 

The admittance, as specified by (1), possesses a constant conductance 
and a susceptance which has a minimum magnitude (zero) at resonance. 
The minimum admittance magnitude therefore occurs at resonance, and 
it is 1/R. Hence, the maximum impedance magnitude is R, and it occurs 
at resonance. 

The maximum value of the response magnitude and the frequency at 


400 Com P lax Frequency 

which it occurs are not always found so easily. In less standard resonant 
circuits, we may find it necessary to express the magnitude of the response 
in analytical form, usually as the square root of the sum of the real part 
squared and the imaginary part squared; then we should differentiate this 
expression with respect to frequency, equate the derivative to zero, solve 
for the frequency of maximum response, and finally substitute this frequency 
into the magnitude expression to obtain the maximum-amplitude response. 
This procedure may be carried out for this simple case merely as a corrob- 
orative exercise, but as we have seen, it is not necessary. 

It should be emphasized that, although the height of the response curve 
of Fig. 14-3 depends only upon the value of R for constant-amplitude 
excitation, the width of the curve or the steepness of the sides depends 
upon the other two element values also. We shall shortly relate the "width 
of the response curve" to a more carefully defined quantity, the bandwidth, 
but it will be helpful to express this relationship in terms of a very important 
parameter, the quality factor Q. 

We shall find that the sharpness of the response curve of any resonant 
circuit is determined by the maximum amount of energy that can be stored 
in the circuit, compared with the energy that is lost during one complete 
period of the response. We define Q as 

„ „ maximum energy stored ,_. 

Q = 2w ; : — __ (5) 

total energy lost per period 

The proportionality constant 2m is included in the definition in order to 
simplify the more useful expressions for Q which we shall now obtain. 
Since energy can be stored only in the inductor and the capacitor, and 
can be lost only in the resistor, we may express Q in terms of the instan- 
taneous energy associated with each of the reactive elements and the 
average power dissipated in the resistor: 

g = 2v K(f) + w c (t)] mBI 


Now let us apply this definition to the parallel RLC circuit and deter- 
mine the value of Q at the resonant frequency. This value of Q is denoted 
by Q . We select the current forcing function 

i(t) = l m cos w t 

and obtain the corresponding voltage response at resonance, 

v(t) = Ri(i) = RI m cos u t 

Then the energy stored in the capacitor is 

401 Frequency Rasponie 

tVcit) = %Cv* = -a|-il cos 2 <V 

The instantaneous energy stored in the inductor becomes 


r 2d2(" 

The total instantaneous stored energy is therefore constant, 

w(t) = w L (t) + w c (t) = S—±. 

and this constant value must also be the maximum value. In order to find 
the energy lost in the resistor in one period, we take the average power 
absorbed by the resistor, 

and multiply by one period, obtaining 

PrT = 4- IJR 
We thus find the quality factor at resonance: 

or Q = 2ir/„fiC = w^C (6) 

Equivalent expressions for Q which are often quite useful may be obtained 
by simple substitution: 

It is apparent that Q is a dimensionless constant which is a function 
of all three circuit elements in the parallel resonant circuit. The concept 
of Q, however, is not limited to electric circuits or even to electrical systems; 
it is useful in describing any resonant phenomenon. For example, let us 
consider a bouncing golf ball. If we assume a weight W and release the 

402 Complex Frequency 

golf ball from a height h x above a very hard (lossless) horizontal surface, 
then the ball rebounds to some lesser height h^. The energy stored initially 
is Wh v and the energy lost in one period is WQi-^ — h^j. The Q is therefore 

Vo (^-/gw h x -h 2 

A perfect golf ball would rebound to its original height and have an infinite 
Q ; a more typical value is 35. It should be noted that the Q in this 
mechanical example has been calculated from the natural response and not 
from the forced response. The Q of an electric circuit may also be de- 
termined from a knowledge of the natural response, as illustrated by 
Prob. 12. 

Let us now relate the various parameters which we have associated 
with a parallel resonant circuit. The three parameters a, co d , and to were 
introduced much earlier in connection with the natural response. Reso- 
nance, by definition, is fundamentally associated with the forced response 
since it is defined in terms of a purely resistive input impedance, a sinusoidal 
steady-state concept. The two most important parameters of a resonant 
circuit are perhaps the resonant frequency <o and the quality factor Q . 
Both the exponential damping coefficient and the natural resonant fre- 
quency may be expressed in terms of co and Q : 

«=--* - - ! - 

2RC 2(Q /u C)C 

■=^ (8) 

and o) d — V"o 2 ~ " 2 

-WH^y (9) 

In terms of these two resonance parameters, the natural response of the 
parallel resonant circuit in the underdamped case 

v(t) = Ae~ at cos u d t 

v(t) = Ae- < ""> /2 «° )( cos con/l -(^T-) 2 ' 

The three critical frequencies (of the input admittance, for example) may 
also be expressed in terms of to and Q . We have the pole at the origin, 

Sj = 

403 frequency Response 

and the pair of conjugate complex zeros, 
h,4= ~ a± i u d 

^-^W 1 -^ 1 

The resonance parameters co and Q may therefore be used to describe 
the natural response in either the time domain or the frequency domain. 
The knowledge provided by these same two parameters about the pole-zero 
constellation also leads to a further interpretation of the settling time and 
the oscillatory behavior of the parallel RLC circuit. For example, we know 
that the settling time, which is the time taken for the natural response to 
"die out," is approximately inversely proportional to a; to the same degree 
of approximation, then, the settling time is directly proportional to Q . 
If both co and Q are increased by the same factor, however, no appreciable 
change in settling time can occur. It is also evident that large values of 
Q cause the natural resonant frequency and the resonant frequency to be 
nearly equal. 

Let us now interpret Q in terms of the pole-zero locations of the 
admittance Y(s) of the parallel RLC circuit. We shall keep <o constant; 
this may be done, for example, by changing R while holding L and C 
constant. As Q is increased, the relationship between a, Q , and <o 
indicates that the two zeros must move closer to the /co axis. The rela- 
tionship between w d , co , and Q shows that the zeros must simultaneously 
move away from the a axis. The exact nature of the movement becomes 
clearer when we remember that the point at which s = jo> could be located 
on the ;co axis by swinging an arc, centered at the origin, through one of 
the zeros and over to the positive /co axis; since <o is to be held constant, 
the radius must be constant, and the zeros must therefore move along this 
arc toward the positive jco axis as Q increases. It is evident that u d and 
co are becoming more nearly equal; if Q is 5, these two frequencies differ 
by about one-half of 1 per cent. 

The "width" of the resonant response curve, such as the one shown 
in Fig. 14-3, may now be defined more carefully and related to Q . Let 
us first define the two half-power frequencies cjj and w 2 as those frequencies 
at which the magnitude of the input admittance of a parallel resonant 
circuit is greater than the magnitude at resonance by a factor of \/2. Since 
the response curve of Fig. 14-3 displays the voltage produced across the 
parallel circuit by a sinusoidal current source as a function of frequency, 
the half-power frequencies also locate those points at which the voltage 
response is 1/ \/5, or 0.707, times its maximum value. A similar relationship 
holds for the impedance magnitude. We shall select co 1 as the lower 
half-power frequency and u 2 as the upper half-power frequency. These 

404 Complex Frequency 

names arise from the fact that a voltage which is 0.707 times the resonant 
voltage is equivalent to a squared voltage which is one-half the squared 
voltage at resonance. 

The (half-power) bandwidth of a resonant circuit is defined as the 
difference of these two half-power frequencies, 

(B = « 2 - w 1 (10) 

We think of this bandwidth as the "width" of the response curve, even 
though the curve actually extends from u = to to = oo. More exactly, 
the half -power bandwidth is measured by that portion of the response curve 
which is equal to or greater than 70.7 per cent of the maximum value. 
Now let us express the bandwidth (B in terms of Q and the resonant 
frequency. In order to do so, we first express the admittance of the parallel 
RLC circuit, 

Y = 


in terms of Q , 

Y = I + ■ 1 ( u "o CR _ "o R ) 
R R\ oi ww L/ 

We note again that the magnitude of the admittance at resonance is 1/fl, 
and then realize that an admittance magnitude of y/2/R can occur only 
when a frequency is selected such that the imaginary part of the bracketed 
quantity has a magnitude of unity. Thus 

Solving, we have 

Ui = (0 r/rwXf_j_] ( i2) 

1 LV \2Q / 2Q i 

^ = "o[/ 1 + (^) 2+ 2^] (13) 

Although these expressions are somewhat unwieldy, their difference pro- 
vides a very simple formula for the bandwidth: 




to 2 

= /(«„ 

+ |«) 

iw d 



s plane 




Fig. 14-4 The pole-zero constellation of Y{s) for a parallel RLC circuit. 
The two zeros are exactly Vi(B Np/s (or rad/s) to the left of the ;u axis and 
approximately ja rad/s (or Np/s) from the a axis. The upper and lower 
half-power frequencies are separated exactly <B rad/s, and each is approxi- 
mately V4CB rad/s away from the resonant frequency and the natural resonant 

= <o, — <o. = ■ 



Circuits possessing a higher £> have a narrower bandwidth, or a sharper 
response curve; they have greater frequency selectivity or higher quality. 
Many resonant circuits are deliberately designed to have a large Q 
in order to take advantage of the narrow bandwidth and high-frequency 
selectivity associated with such circuits. When Q is larger than about 5, 
it is possible to make some very useful approximations in the expressions 
for the upper and lower half-power frequencies and in the general expres- 
sions for the response in the neighborhood of resonance. Let us arbitrarily 
refer to a high-Q circuit as one in which Q is equal to or greater than 
5. The pole-zero configuration of Y(s) for a parallel RLC circuit having 
a Q of about 5 is shown in Fig. 14-4. Since 


a = %(B 


406 Complex Frequency 

and the locations of the two zeros may be approximated: 

s 2,4- -y 2 ® ±k 

Moreover, the locations of the two half-power frequencies (on the positive 
ju axis) may also be determined in a concise approximate form: 

or <o 12 = «„ + V 2 (B (15) 

In a high-@ circuit, therefore, each half-power frequency is located ap- 
proximately one-half bandwidth from the resonant frequency; this is in- 
dicated in Fig. 14-4. 

Now let us visualize a test point slightly above /«„ on the /to axis. In 
order to determine the admittance offered by the parallel RLC network 
at this frequency, we construct the three vectors from the critical frequen- 
cies to the test point. If the test point is close to /(o , then the vector from 
the pole is approximately /co and that from the lower zero is nearly /2to . 
The admittance is therefore given approximately by 

¥(s) = c 0HX'-»J ^ 2C(S _ S2) ( i6) 

where the multiplicative constant C is determined from (4). In order to 
determine a useful approximation for the vector (s - s 2 ), let us consider 
an enlarged view of that portion. of the s plane in the neighborhood of 
the zero % (Fig. 14-5). We define the angle of the admittance as 9 Y , 

and note from (16) that Y may also be identified approximately as the angle 
of s — S2. Thus 



s - s 2 = y 2 (B + /y 2 (B tanfiy = %(B(1 + / tan0 y ) 
s - s 2 = y 2 <BVl-Man 2 y /By 

Y(s) = 2C(y 2 (B) Vl + tan 2 y ftr 

Y(s) = iVl + tan 2 «;/ffy (17) 

: tan %« 


r'a> <approx.) 

Fig. 14-5 An enlarged portion of the pole-zero constellation for Y(s) of 
a high-^) parallel RLC circuit. 

Thus, the angle of the admittance at a given frequency near resonance 
is obtained by calculating the number of half bandwidths by which the 
frequency is off resonance and then taking the inverse tangent of this 
number; being careful to preserve the algebraic sign. The magnitude of 
the admittance at this frequency is given approximately by the product of 
the conductance 1/R and the square root of one plus the square of the 
number of half bandwidths off resonance. 

As an example of the use of these approximations, let us determine the 
approximate value of the admittance of a parallel RLC network for which 
R = 25 kfi,L = 1 H,andC = ]/ 25 fiF. Wenndthatg> = 5,co = 5 krad/s, 
(B = 1 krad/s, and (B/2 = 0.5 krad/s. Let us evaluate the admittance at 
<o = 5.25 krad/s, a frequency which is one-half of a half bandwidth above 
resonance. Thus, 

B Y ~ tan- 1 (0.5) = 26.6° 

and Y(/5250) = 0.04 Vl + ffl.5) 2 /26.6° = 0.0447 /26.6° mZ5 

An exact calculation of the admittance shows that 

Y(/5250) = 0.0445 /26.0° mW 

The approximate method therefore leads to values of admittance magni- 
tude and angle that are too high by about 0.5 and 2 per cent, respectively. 
Our intention is to use these approximations for high-() circuits near 
resonance. We have already agreed that we shall let "high-^)" infer 
Q > 5, but how near is "near"? It can be shown that the error in magni- 
tude or phase is less than 5 per cent if Q > 5 and 0.9« < to < l.lto . 


408 Comptox Frequency 

Although this narrow band of frequencies may seem to be prohibitively 
small, it is usually more than sufficient to contain the range of frequencies 
in which we are most interested. For example, a home radio may contain 
a circuit tuned to a resonant frequency of 455 kHz with a half-power 
bandwidth of 10 kHz. This circuit must then have a value of 45.5 for Q , 
and the half-power frequencies are about 450 and 460 kHz. Our approxi- 
mations, however, are valid from 409.5 to 500.5 kHz (with errors less than 
5 per cent), a range which covers essentially all the peaked portion of the 
response curve; only in the remote "tails" of the response curve do the 
approximations lead to reasonably large errors. 1 

Let us conclude our coverage of the parallel resonant circuit by re- 
viewing the various conclusions we have reached. The resonant frequency 
o> is the frequency at which the imaginary part of the input admittance 
becomes zero or the admittance angle 8 Y becomes zero. Then, to = 
1/ y/LC. The circuit's figure of merit Q is defined as 2w times the ratio 
of the maximum energy stored in the circuit to the energy lost each period 
in the circuit. From this definition, we find that Q = coqRC. The two 
half-power frequencies u 1 and to, are defined as the frequencies at which 
the admittance magnitude is V2 times the minimum admittance magni- 
tude. These are also the frequencies at which the voltage response is 70.7 
per cent of the maximum response. The exact and approximate (for high 
Q ) expressions for these two frequencies are 

where ffi is the difference between the upper and the lower half-power 
frequencies. This half-power bandwidth is given by 


The input admittance may also be expressed in an exact or approximate 
(for high Q ) form 

Y = 1 VI + tan»g y /g y = jjl + (^y^f Aan- 1 [(<■> - «.„)/%«] 

The approximations are valid for frequencies which do not differ from the 
resonant frequency by more than one-tenth of the resonant frequency. 

*At frequencies remote from resonance, we are often satisfied with very rough results; greater 
accuracy is not always necessary. 

409 Frequency Response 

Drill Problems 

14-1 Determine <o for the parallel resonant circuit described by: (a) L = % 2 H, 
C = 3 iiF, R = 1 kQ; (b) a = 40,000 s" 1 , fi = 100 kfl, L = 80 fiH; (c) u t = 
100 v^T s" 1 , C = 20 fiF, a = 200 s" 1 . 

Ans. 500; 2000; 10,000,000 rad/s 

14-2 Find Q for each of the networks described in Drill Prob. 14-1. 

Ans. 1.25; 6; 125 

1 4-3 Specify the locations of the zeros of Y(s) for a parallel RLC circuit for which: 
(a) Q = 5, L = 0.4 H, C = 10 jkF; (b) Q = 4, <o = 480 rad/s, R = 172 Q; 
(J) Q = 3, R = 500 Q, C = 20 juF. 

Ans. -50 ± j296; -50 ± j498; -60 ± j476 s" 1 

14-4 Find (B, u lt and o> 2 for the parallel RLC circuit of Drill Prob. 14-3: (a) 

la; (b) lb; (c) lc. 

Ans. 400, 339, 739; 333, 1840, 2174; 8 X 10*, 9.96 X 10 6 , 10.04 X 10 6 rad/s 

14-5 Given a parallel circuit, R = 100 £2, L = 5 mH, C = 50 ^F, and a current 
source, i s = 0.01 cos ut A, find the amplitude of the capacitor voltage if a = : 
(a) 2000; (b) 1850; (c) 2120 rad/s. 

An*. 0.55; 0.64; 1.00 V 


Although we probably find less use for the series RLC circuit than we do 
for the parallel RLC circuit, it is still worthy of our attention. We shall 
consider the circuit shown in Fig. 14-6. It should be noted that the various 
circuit elements are given s (for series) subscripts for the time being in 
order to avoid confusing them with the parallel elements when the circuits 
are to be compared 

Our discussion of parallel resonance required a section of considerable 
length. We could now give the series RLC circuit the same kind of treat- 
Fig. 14-6 A series resonant circuit. 

i — V*A njw- 



410 Complex Frequency 

ment, but it is much cleverer to avoid such needless repetition and use 
the duality principle. For simplicity, let us concentrate on the conclusions 
presented in the last paragraph of the preceding section on parallel reso- 
nance. The important results are contained there, and the use of dual 
language enables us to transcribe this paragraph to present the important 
results for the series RLC circuit. 

Let us conclude our coverage of the series resonant circuit by sum- 
marizing the more important conclusions. The resonant frequency co 0s is 
the frequency at which the imaginary part of the input impedance becomes 
zero or the impedance phase angle Z becomes zero. Then, to 0g = 
1/ V-L S C S . The circuit's figure of merit Q 0s is defined as 2ot times the ratio 
of the maximum energy stored in the circuit to the energy lost each period 
in the circuit. From this definition, we find that Q 0s = oi 0s L s /R s . The two 
half-power frequencies co ls and <c 2s are defined as the frequencies at which 
the impedance magnitude is a/2 times the minimum impedance magnitude. 
These are also the frequencies at which the current response is 70.7 per 
cent of the maximum response. The exact and approximate (for high Q 0s ) 
expressions for these two frequencies are 

where (B s is the difference between the upper and the lower half-power 
frequencies. This half-power bandwidth is given by 

<B, = to, 

u 0j 




The input impedance may also be expressed in an exact or approximate 
(for high QJ form 

Z s = H.Vl + tan»«,^, = R,Jl + (^y£f) /tan" 1 [(« - a. J/%«.] 

The approximations are valid for frequencies which do not differ from the 
resonant frequency by more than one-tenth of the resonant frequency. 

The series resonant circuit is characterized by a low impedance at 
resonance, while the parallel resonant circuit produces a high resonant 
impedance. The latter circuit provides inductor currents and capacitor 
currents at resonance which have amplitudes Q times as great as the source 
current; the series resonant circuit provides inductor voltages and capacitor 
voltages which are greater than the source voltage by the factor Q 0s . 

From this point on, we shall no longer identify series resonant circuits 
by use of an $ subscript. 

411 Frequency Response 

Drill Problems 

1 4-6 Find the half-power bandwidth and the Q of a series RLC circuit contain- 
ing: (a) R=z2Q, L=10mH, C=100juF; (b) R = 25 Q, L = 50 mH, 
C = 20 nF; (c) R = 10 Q, L = 0.2 H, C = 5/iF. 

An*. 50 rad/s, 20; 200 

rad/s, 5; 500 rad/s, 2 

1 4-7 Let each network described in Drill Prob. 6 be excited by the forcing func- 
tion 2 cos at V. Find the magnitude of the capacitor voltage at u = 960 rad/s. 

Ans. 4.1; 9.6; 21.8 V 


The parallel and series RLC circuits of the previous two sections represent 
idealized resonant circuits; they are no more than useful approximate 
representations of a physical circuit which might be constructed by com- 
bining a coil of wire, a carbon resistor, and a tantalum capacitor in parallel 
or series. The degree of accuracy with which the idealized model fits the 
actual circuit depends on the operating frequency range, the Q of the 
circuit, the materials present in the physical elements, the element sizes, 
and many other factors. We are not studying the techniques of determining 
the best model for a given physical circuit, for this requires some knowledge 
of electromagnetic field theory and the properties of materials; we are, 
however, concerned with the problem of reducing a more complicated 
model to one of the two simpler models with which we are more familiar. 
The network shown in Fig. 14-7a is a reasonably accurate model for 
the parallel combination of a physical inductor, capacitor, and resistor. 
The resistor Rj represents the ohmic losses, core losses, and radiation losses 
of the physical coil. The losses in the dielectric within the physical capaci- 
tor are accounted for by the resistor R 2 , as well as for the resistance of 

Fig. 14-7 (a) A useful model of a physical network which consists of a 
physical inductor, capacitor, and resistor in parallel, [b) A network which can 
be equivalent to (a) over a narrow frequency band. 


412 Complex Frequency 

the physical resistor in the given RLC circuit. In this model, there is no 
way to combine elements and produce a simpler model which is equivalent 
to the original model for all frequencies. We shall show, however, that 
a simpler equivalent may be constructed which is valid over a frequency 
band which is usually large enough to include all frequencies of interest. 
The equivalent will take the form of the network shown in Fig. l4-7b. 
Before we learn how to develop such an equivalent circuit, let us first 
consider the given circu it, F ig. 1A-Ia. The resonant radian frequency for 
this network is not 1/ vLC, although if R 1 is sufficiently small it may be 
very close to this value. The definition of resonance is unchanged, and 
we may determine the resonant frequency by setting the imaginary part 
of the input admittance equal to zero: 

tomw] = fa (i + ^ + _i_ : ) SB o 



C = 

V + u 2 L? 

^ U " = J^-(f) 2 

We note that w is less than 1/\LC, but sufficiently small values of the 
ratio RJL may result in a negligible difference between w and 1/ yj~L£. 
The maximum magnitude of the input impedance also deserves consid- 
eration. It is not R 2 , and it does not occur at <o (or at o> = 1/ y/LC). The 
proof of these statements will not be shown because the expressions soon 
become algebraically cumbersome; the theory, however, is straightforward. 
Let us be content with a numerical example. We select the simple values 
R 1 = 2 a, L = 1 H, C = % F, and R 2 = 3 fl, and find the resonant fre- 

w = 2 rad/s 
and the input impedance at resonance 

Z(/2) = 1.714 Q 
At the frequency which would be the resonant frequency if R 1 were zero, 

= 2.83 rad/s 

the input impedance is 

Z(/2.83) = 1.94 7/- 13.26° Q 




o— — 


} — *■■ * 

► H » 

/x p 



Fig. 14-8 (a) A series network which consists of a resistance R a and an 
inductive or capacitive reactance X, may be transformed into (b) a parallel 
network such that Y 8 = Y p at one specific frequency. The reverse trans- 
formation is equally possible. 

However, the frequency at which the maximum impedance magnitude 
occurs, indicated by « m , is found to be 

<o m = 3.26 rad/s 

and the impedance having the maximum magnitude is 

Z(/3.26) = 1.98 /-21.4° Q 

The impedance magnitude at resonance and the maximum magnitude differ 
by about 13 per cent. Although it is true that such an error may be 
neglected occasionally in practice, it is too large to neglect on a test. The 
later work in this section will show that the Q of the inductor-resistor 
combination at 2 rad/s is unity; this low value accounts for the 13 per 
cent discrepancy. 

In order to transform the given circuit of Fig. 14-7a into an equivalent 
of the form of that shown in Fig. 14-7b, we must discuss the Q of a simple 
series or parallel combination of a resistor and a reactor (inductor or 
capacitor). We first consider the series circuit shown in Fig. 14-8a. The 
Q of this network is again defined as 2ir times the ratio of the maximum 
stored energy to the energy lost each period, but the Q may be evaluated 
at any frequency we choose. In other words, Q is a function of to. It is 
true that we shall choose to evaluate it at a frequency which is, or ap- 
parently is, the resonant frequency of some network of which the series 
arm is a part. This frequency, however, is not known until a more complete 
circuit is available. The eager reader is encouraged to show that the Q 
of this series arm is \X a \/R s , whereas the (? of the parallel network of Fig. 
14-8fc is R P /\X„\. 

Let us now carry out the details necessary to find values for R p and 
X p so that the parallel network of Fig. 14-8& is equivalent to the series 
network of Fig. 14-8a at some single specific frequency. We equate Y s 
and Y p , 


414 Complex Frequency 

1 R, -jX, 1 


• fi 8 + /X s R* + X* ' R p 


and obtain 

Dividing these two expressions, we find 

r p X s 
x. R, 

It follows that the Q's of the series and parallel networks must be equal: 

Qp = ft = Q 
The transformation equations may therefore be simplified: 

R p = «.(1 + p 2 ) (19) 

— y l i j , 

*» = X .( 1 + ^) («>) 

It is apparent that R s and X s may also be found if R p and X p are the given 
values; the transformation in either direction may be performed. 

If Q> 5, little error is introduced by using the approximate rela- 

Rp = Q 2 R S (21) 

X p = X„ (C p = C s or L p = L,) (22) 

As an example, consider the series combination of a 100-mH inductor 
and a 5-0 resistor. We shall perform the transformation at a frequency 
of 1000 rad/s, a value selected because it is approximately the resonant 
frequency of the network (not shown) of which this series arm is a part. 
We find that X a is 100 to and Q is 20. Since the Q is sufficiently high, 
we use (21) and (22) to obtain 

R p = (^R, = 2000 B L p = L s = 100 mH 

The conclusion is that a 100-mH inductor in series with a 5-Q resistor 
provides essentially the same input impedance as does a 100-mH inductor 
in parallel with a 2000-0 resistor at the frequency 1000 rad/s. In order 
to check the accuracy of the equivalence, let us evaluate the input im- 
pedance for each network at 1000 rad/s. We find 

415 Frequency Responw 

Z s (/1000) = 5 + /100 = 100.1 /87.1° 

7 (/1 Q00) = 200 °<' 100) = 99.9/87.1° 
p(1 ' 2000 + ;100 L 

and conclude that the approximation is exceedingly accurate at the trans- 
formation frequency. The accuracy at 900 rad/s is also reasonably good, 

Z s (/900) = 90.1 /86.8° 
Z p (/900) = 89.9 /87.4° 

If this inductor and series resistor had been used as part of a series RLC 
circuit for which the resonant frequency was 1000 rad/s, then the half- 
power bandwidth would have been 

^ = i ooo = 

Q 20 

and the frequency of 900 rad/s would have represented a frequency that 
was 4 half bandwidths off resonance. Thus the equivalent networks that 
we evaluated above would have been adequate for reproducing essentially 
all the peaked portion of the response curve. 

As a further example of the replacement of a more complicated resonant 
circuit by an equivalent series or parallel RLC circuit, let us consider a 
problem in electronic instrumentation. The simple series RLC network in 
Fig. 14-9a is excited by a sinusoidal voltage source at the resonant fre- 
quency. The effective value of the source voltage is 0.5 V, and we wish 
to measure the effective value of the voltage across the capacitor with an 
electronic voltmeter (VM) having an internal resistance of 100,000 S2. That 
is, an equivalent representation of the voltmeter is an ideal voltmeter in 
parallel with a 100,000-fi resistor. 

Before the voltmeter is connected, we find that the resonant frequency 
is 10 5 rad/s, Q = 50, the current is 25 mA, and the rms capacitor voltage 
is 25 V. As indicated at the end of Sec. 14-3, this voltage is Q times the 
applied voltage. Thus, if the voltmeter were ideal, it would read 25 V 
when connected across the capacitor. 

However, when the actual voltmeter is connected, the circuit shown 
in Fig. 14-9b results. In order to obtain a series RLC circuit, it is now 
necessary to replace the parallel RC network by a series RC network. Let 
us assume that the Q of this RC network is sufficiently high so that the 
equivalent series capacitor will be the same as the given parallel capacitor. 
We do this in order to approximate the resonant frequency of the final 
series RLC circuit. Thus, if the series RLC circuit also contains a 0.01-/iF 
capacitor, the resonant frequency remains 10 5 rad/s. We need to know 

20 a 10 mH 

100 kfl 

loo kn 

Fig. 14-9 (a) A given series-resonant circuit in which the capacitor voltage 
is to be measured by a nonideal electronic voltmeter, (b) The effect of the 
voltmeter is included in the circuit; it reads V' c volts, (c) A series resonant circuit 
is obtained when the parallel RC network in [b) is replaced by the series RC 
network which is equivalent at 10 5 rad/s. 

this estimated resonant frequency in order to calculate the Q of the parallel 
RC network; it is 

Q = 


wR p C p = io^io^io- 8 ) = 100 

Since this value is greater than 5, our vicious circle of assumptions is 
justified, and the equivalent series RC network consists of the capacitor 

and the resistor 

C, = 0.01 juF 

fl 8 = ^=10 Q 

Hence, the equivalent circuit of Fig. 14-9c is obtained. The resonant Q 
of this circuit is now only 33.3, and thus the voltage across the capacitor 
in the circuit of Fig. 14-9c is 16y 3 V. But we need to find |V^|, the voltage 
across the series RC combination; we obtain 

|VJ| =^-|10-/1000| = 16.7 V 


4|7 frxiuMKy Response 

The capacitor voltage and | V c \ are essentially equal since the voltage across 
the 10-8 resistor is quite small. 

The final conclusion must be that an apparently good voltmeter may 
produce a severe effect on the response of a high-Q resonant circuit. A 
similar effect may occur when a nonideal ammeter is inserted in the circuit. 

Drill Problems 

14-8 Given a 10-fl resistor in series with a 10-juF capacitor, determine the 
two-element parallel equivalent if u = : (a) 200; (b) 1000; (c) 5000 rad/s. 

Ans. 50 fl, 8 nF; 1 fcQ, 10 juF; 25 fcQ, 10 jiF 

14-9 At <o = 10 3 rad/s, find the effective Q of the two-terminal RC networks 
shown in Fig. 14- 10a, b, and c. 

Ans. 2; 10; 20 



(a) (b) 

Fig. 14-10 See Drill Prab. 14-9. 

14-10 A certain physical inductor is modeled by an ideal 10-mH inductor in 
series with a 10-S2 resistor, while a capacitor is approximated by an ideal y 9 -fiF 
capacitor in series with 5 Q. If the two physical elements are connected in 
parallel, find the approximate: (a) parallel resonant frequency; (b) lower half-power 
frequency; (c) upper half-power frequency. 

Ans. 29,250; 30,000; 30,750 rad/s 


Some of the examples and problems which we have been solving have 
involved circuits containing element values ranging around a few ohms, 
a few henrys, and a few farads. The applied frequencies were a few radians 
per second. These particular numerical values were used not because they 
are those commonly met in practice, but because arithmetic manipu- 
lations are so much easier than they would be if it were necessary to carry 
along various powers of 10 throughout the calculations. The scaling pro- 
cedures that will be discussed in this section enable us to analyze networks 
composed of practical-sized elements by scaling the element values to 



0) (rad/s) 


Fig. 14-11 [a) A parallel resonant circuit used as an example to illustrate 
magnitude and frequency scaling, [b) The magnitude of the input impedance 
is shown as a function of frequency. 

permit more convenient numerical calculations. We shall consider both 
magnitude scaling and frequency scaling. 

Let us select the parallel resonant circuit shown in Fig. 14-lla as our 
example. The impractical element values lead to the unlikely response 
curve drawn as Fig. 14-1 lb; the maximum impedance is 2.5 £2, the resonant 
frequency is 1 rad/s, Q is 5, and the bandwidth is 0.2 rad/s. These 
numerical values are much more characteristic of the electrical analog of 
some mechanical system than they are of any basically electrical device. 
We have convenient numbers with which to calculate but an impractical 
circuit to construct. 

Let us assume that our goal is to scale this network in such a way as 
to provide an impedance maximum of 5000 £2 at a resonant frequency of 
5 X 10 6 rad/s, or 796 kHz. In other words, we may use the same response 
curve shown in Fig. 14-11& if every number on the ordinate scale is 
increased by a factor of 2000 and every number on the abscissa scale is 
increased by a factor of 5 X 10 6 . We shall treat this as two problems: (1) 
scaling in magnitude by a factor of 2000 and (2) scaling in frequency by 
a factor of 5 X 10 6 . 

Magnitude scaling is denned as the process by which the impedance 
of a two-terminal network is increased by a factor of K m , the frequency 
remaining constant. The factor K m is real and positive; it may be greater 
or smaller than unity. We shall understand that the shorter statement, "the 
network is scaled in magnitude by a factor of 2," infers that the impedance 
of the new network is to be twice that of the old network at any frequency. 
Let us now determine how we must scale each type of passive element. 
To increase the input impedance of a network by a factor of K m , it is 
sufficient to increase the impedance of each element in the network by 
this same factor. Thus, a resistor R must be replaced by a resistor K m R. 
Each inductor must also exhibit an impedance which is K m times as great 



jlOOOH =t=10 









-— ^^ i 

1 1 1 > 




2 a) (rad/s) 

Fig. 14-12 (a) The network of Fig. 1 4-1 1 a after being scaled in magnitude 
by a factor K m = 2000. (b) The corresponding response curve. 

at any frequency. In order to increase an impedance sL by a factor of 
K m when s remains constant, the inductor L must be replaced by an inductor 
K m L. In a similar manner, each capacitor C must be replaced by a capacitor 
C/K m . In summary, these changes will produce a network which is scaled 
in magnitude by a factor of K m : 

R ^ K m R^ 
L-> K m L 

magnitude scaling 

When each element in the network of Fig. 14-1 la is scaled in magnitude 
by a factor of 2000, the network shown in Fig. 14- 12a results. The response 
curve shown in Fig. 14-12& indicates that no change in the previously drawn 
response curve need be made other than a change in the scale of the 

Let us now take this new network and scale it in frequency. We define 
frequency scaling as the process by which the frequency at which any 
impedance occurs is increased by a factor of K f . Again, we shall make 
use of the shorter expression, "the network is scaled in frequency by a factor 
of 2," to infer that the same impedance is now obtained at a frequency 
twice as great. Again, frequency scaling is accomplished by scaling each 
passive element in frequency. It is apparent that no resistor is affected 
The impedance of any inductor is sL, and if this same impedance is to 
be obtained at a frequency K f times as great, then the inductor L must 
be replaced by one having an inductance of L/K f . Similarly, a capacitor 
C is to be replaced by one having a capacitance C/K f . Thus, if a network 
is to be scaled in frequency by a factor of K f , then the changes necessary 
in each passive element are 


Z'— *- <5kfl 

J200/1H q=200pF 


5 7.5 

<«) (6) 

Fig, 14-13 (a) The network of Fig. 1 4-1 2c after being seated in frequency 
by a factor K f == 5 X 10 6 . \b) The corresponding response curve. 

10 <j) (Mrad/s) 



frequency scaling 

When each element of the magnitude-scaled network of Fig. 14-12o is 
scaled in frequency by a factor of 5 X 10 6 , the network of Fig. 14- 13a 
is obtained. The corresponding response curve is shown in Fig. 14-13fo. 

The circuit elements in this last network have values which are easily 
achieved in physical circuits; the network can actually be built and tested. 
It follows that, if the original network of Fig. 14-1 la were actually an 
analog of some mechanical resonant system, we could have scaled this 
analog in both magnitude and frequency in order to achieve a network 
which we might construct in the laboratory; tests that are expensive or 
inconvenient to run on the mechanical system could then be made on the 
scaled electrical system, and the results should then be "unsealed" and 
converted into mechanical units to complete the analysis. 

The effect of magnitude scaling or frequency scaling on the pole-zero 
constellation of an impedance is not very difficult to ascertain, but its 
determination offers such an excellent opportunity to review the meaning 
and significance of a pole-zero plot in the s plane that it forms the basis 
for one of the drill problems below. 

An impedance which is given as a function of s may also be scaled 
in magnitude or frequency, and this may be done without any knowledge 
of the specific elements out of which the two-terminal network is com- 
posed. In order to scale Z(s) in magnitude, the definition of magnitude scaling 
shows that it is only necessary to multiply Z(s) by K m in order to obtain the 
magnitude-scaled impedance. Thus, the impedance of the parallel resonant 
circuit shown in Fig. 14-1 la is 


421 Frequancy RciponM 


'. 2s 2 + 0.4s + 2 
Z(s) = 0.5- 

(s + 0.1 + /0.995)(s + 0.1 - /0.995) 

The impedance Z'(s) of the magnitude-scaled network is 

Z'(i) = K m Z(s) 
and, therefore, 

Z'(s) = 1000- 

(s + 0.1 + ;0.995)(s + 0.1 - /0.995) 

If Z'(s) is now to be scaled in frequency by a factor of 5 X 10 6 ; then Z"(s) 
and Z'(s) are to provide identical values of impedance if Z"(s) is evaluated 
at a frequency K f times that at which Z'(s) is evaluated. After some careful 
cerebral activity, this conclusion may be stated concisely in functional no- 

it) = z ' (s) 

Remember that the correspondence results when a larger value of s is used 
in Z" (assuming that K f > 1). In other words, we obtain Z"(s) by replacing 
every s in Z'(s) by s/K f . The analytic expression for the impedance of the 
network shown in Fig. 14-13a must therefore be 

Z »/ $) = 100 s /( 5 X 1Q6 ) 

v ' [s/(5 X 10 6 ) + 0.1 + /0.995][s/(5 X 10 6 ) + 0.1 - /0.995] 


X"(s) = 5 y 10 9 - 

w ^ (s + 0.5 X 10 6 + /4.975 X 10 6 )(s + 0.5 X 10 6 - /4.975 X 10 6 ) 

Drill Problems 

14-11 A parallel resonant circuit has a resonant frequency of 2500 rad/s, a 
bandwidth of 100 rad/s, and an inductance of 200 mH. Find the new bandwidth 
and capacitance if the circuit is scaled: (a) in magnitude by a factor of 5; (b) 
in frequency by a factor of 5; (c) in magnitude and frequency by factors of 5. 
Am. 100 rad/s, 0.16 ixF; 500 rad/s, 0.032 /iF; 500 rad/s, 0.16 pF 

14-12 A scaled series resonant circuit consists of a 2-fi resistor, a 5-H inductor, 
and a 0.8-F capacitor. Find K m and K f if the original circuit contained a: (a) 

422 Complex Frequency 

50-0 resistor and a I6-/1F capacitor; (b) 50-J2 resistor and a 1-H inductor; (c) 
1-H inductor and a 16-jxF capacitor. 

Ans. 10~ 2 , 2 X 10~ 3 ; 4 X 10~ 2 , 5 X 10~ 4 ; 4 x 10' 2 , 8 X 10~ 3 

14-13 The magnitude of an admittance has been modeled on the s plane by 
an elastic sheet, as described in Sec. 13-7. The height of the sheet above the origin 
is 28 cm, and the location of a certain zero is 40 cm distant from the origin in a 
direction 1 10 ° counterclockwise from the 4- axis. Find the distance, direction, and 
height if the admittance is scaled by: (a) K m = 2, K f = 1; (b) K m = 1, K, = 2; (c) 
K m = 2,K f = 2. 

Ans. 40 cm, 110°, 56 cm; 80 cm, 110°, 28 cm; 80 cm, 110°, 56 cm 

14-14 A voltage Vj(s) applied to a given network produces an output response 
I 2 (s) = (2s + 5)/(3s 2 + 4s + 6) A. Find I 2 (s) if the network is scaled in: (a) 
frequency by a factor of 2; (b) magnitude by a factor of 2; (c) frequency and 
magnitude by factors of 2. 

s + 2.5 4s + 20 2s + 20 


3s 2 + 4s + 6 ' 3s 2 + 8s + 24 ' 3s 2 + 8s + 24 


D 1 A parallel network contains R = 1 Ml, L = y i2 H, and C = % /iF. Find co , 
/o> Qo< a < u d< an d th e locations of the impedance poles. 

□ 2 If the independent current source, 6 cos u t mA, is connected to the network 
described in Prob. 1, find V, I R , l L , I c , P K , w L (t), w c (t), and the ratios of |IJ and 
|I C | to the source current amplitude. 

□ 3 Find the values of the three elements comprising a parallel resonant circuit 
if: (a) Q = 10, L = 2 H, R = 2 kfi; (b) W = 0.2 J, C = 0.1 fiF, co = 2000 rad/s, 
Pbo = 400 W. 

D 4 A parallel resonant circuit exhibits a natural response in which successive 
positive maxima have a ratio of 0.99 and the zero crossings are 0.4 ms apart. 
Find a, u d , io , and Q . 

D 5 If w = 1 krad/s in a parallel resonant circuit, find Q if the lower half-power 
frequency is: (a) 0.99 krad/s; (b) 0.8 krad/s; (c) 0.1 krad/s. 

□ 6 A parallel resonant circuit driven by a current source, 0.2 cos wt A, shows a 
maximum voltage response amplitude of 80 V at u = 2500 rad/s and 40 V at 
2200 rad/s. Find R, L, C, Q , and the half-power frequencies. 

D 7 Measurements on a pendulum making one complete swing every 1.6 s indicate 
that the oscillation amplitude drops to 50 per cent of its initial value in 2 min. 
What is the Q ? 

423 Frequency Response 

□ 8 Sketch a curve of |V| versus <o for the circuit shown in Fig. 14-14 if u = 
10 4 rad/s and C = : (a) 1 /iF; (&) 0.1 fiF. 


Fig. 14-14 See Probs. 8 and 9. 

□ 9 Find <o 0> g , <B, and V at <o = co in the circuit shown in Fig. 14-14 if C = 2 M F, 
L = 5 mH, and there is a 500-& resistor placed in parallel with the capacitor. 

D 10 A voltage source V, is in series with a series RLC network, (a) Show that 
maximum am plitude of the capacitor voltage is <? |V,|/ \A - 1/(4C" 2 ) and that J 1 
occurs at <o Vl - l/(2<? 2 )- ( b ) Show that the ma5dmunl ind uctor voltage equals 
the maximum capacitor voltage, but that it occurs at <o /Vl - l/(2C- 2 ). 

□ 1 1 Find Q , co 0> Wl , co 2 , and <B for a series RLC network in which: (a) R = 8 a, 
L = 0.02 H, C = 0.5 M F; (b) R = 400 fi, L = 0.2 H, C = 5 /iF. 

D 12 The C- of a series or parallel RLC network may be obtained by applying 
the definition of Q to the natural response. For example, assume a high-C- series 
circuit and a natural response of the form i(f) = /„«-" cos<o d t. Determine the 
stored energy at t = and t = 2*/w d = 2v/o> , the time at which i has its first 
maximum after t = 0. From these facts, find Q . 

□ 13 A two-terminal network has an impedance whose pole-zero constellation is 
shown in Fig. 14-15. If the minimum impedance magnitude at any radian 
frequency is 72 fi, find the magnitude of the impedance at: (a) <o = 4000; 
(b) o= = 3600; (c) <o = 8000; (d) s = -200 + JO; (e) s = -200 + /200 s \ 

Fig. 14-15 See Prob. 13. 




O - -/4000 

424 Complajf Frequency 

D 14 A voltage source, 2 cos ut V, is available and a current response as a function 
of frequency is desired that has a maximum of 2 mA at <o = 10 5 rad/s and falls 
off to v2 mA at 2000 rad/s above or below a> . Design a series resonant circuit to 
do this. 

D 1 5 The circuit shown in Fig. 14-16 is a simplified example of a Q meter. A 
physical inductor, which we represent as a resistor R L in series with an inductor 
L, is mounted between terminals a-b. The capacitor is adjusted to maximize |V C |. 
What restrictions must be placed on R L and L in order that |V c | in mV = Q = 
UqL/R l with less than 1 per cent error? 

a b 

T O o 

25 mA 

Fig. 14-16 See Prob. 15. 

D 16 A source V cos at is applied to a high-Q RLC series network. Assume that 
an ideal voltmeter can be connected across L and C in series (but not R), and 
sketch |V iC | versus «. Indicate <o , u v w 2 , and V on the sketch and specify the 
shape of the curve near oi = w . 

D 17 For the circuit shown in Fig. 14-17, determine the resonant frequency, the 
Q , the bandwidth, and sketch |I| versus w. What would the Q of the circuit 
be if the 20-fi resistor were short-circuited? Or if the 200-kJ2 resistor were 


20 a 0.2 H 
10/0° v(£) 200 kO 

Fi 9 . 14-17 See Prob. 17. 

□ 18 Determine the maximum amplitude of the capacitor voltage in the circuit 
shown in Fig. 14-18, the frequency at which it occurs, and indicate by a simple 
sketch its variation with frequency near resonance, near o> = 0, and as o) 
approaches infinity. 

Fig. 14-18 See Prob. 18. 


15 $2 

40 H2 


425 Frequency Response 

D 19 A 0.01-/iF capacitor having an effective series resistance of 20 Q is placed 
in parallel with a 10-mH inductor having an effective series resistance of 10 fl. 
Two other parallel elements, a 5-mA sinusoidal current source and a 300-kfl 
resistor, complete the circuit. Describe the variation of the voltage across the 
source as a function of frequency. 

D 20 As an indication of the fact that active elements may be used to increase 
the Q of resonant circuits, find Q for the circuit shown in Fig. 14-19 by an 
inspection of the input admittance presented to the independent source if k = : 
(a) 0; (b) 4 X lO" 5 ; (c) -2 X 10~ 4 . 

Fi 9 . 14-19 See Prob. 20. 

□ 21 (a) Express the resonant frequency and Q of the network shown in Fig. 14-20 
as functions of R, L, C, and k. (b) Repeat if the positions of R and C are inter- 




Fig. 14-20 See Prob. 21. 

□ 22 (a) If the network shown in Fig. 14-21 is excited by a forcing function 
V m cos ut, determine the source current at u = 0, 1, 11, 12, 13, and 30 rad/s and 
sketch the current amplitude as a function of to, < w < 30. Check your results 
by approximate methods, (b) If the forcing function is V u(t), find the source 
current as a function of time and sketch the current as a function of time, 

14-21 See Probs. 22 and 23. 

□ 23 Refer to the circuit shown in Fig. 14-21 and scale it: (a) in magnitude so 
that L = 2 mH; (b) in frequency so that L = 2 mH; (c) in magnitude and fre- 
quency so that L = 2 mH and C = 0.2 /iF. 

426 Complex Frequency 

□ 24 A parallel resonant circuit in which R = 60 left has w = 2 X 10 5 rad/s and 
Q = 80. Find the new element values after the circuit is scaled so that R' = 1 $2, 
and u' = 1 rad/s. 

D 25 A series resonant circuit in which a = 2, <J d = 30 s" 1 , and L = 20 H is scaled 
in such a way that a becomes 10 3 s _1 while the new capacitance is 0.01 /iF. 
Determine the new element values. 

Chapter Fifteen 




Several hundred pages ago the inductor was introduced as a circuit element 
and defined in terms of the voltage across it and the time rate of change 
of the current through it Strictly speaking, our definition was of "self- 
inductance," but, loosely speaking, "inductance" is the commonly used 
term. Now we need to consider mutual inductance, a property which is 
associated mutually with two or more coils which are physically close 
together. A circuit element called the "mutual inductor" does not exist; 
furthermore, mutual inductance is not a property which is associated with 
a single pair of terminals, but instead is defined with reference to two pairs 
of terminals. 

432 ^wo^P ** Network* 

Mutual inductance results through the presence of a common magnetic 
flux which links two coils. It may be defined in terms of this common 
magnetic flux, just as we might have defined self-inductance in terms of 
the magnetic flux about the single coil. However, we have agreed to confine 
our attention to circuit concepts, and such quantities as magnetic flux and 
flux linkages are mentioned only in passing; we cannot define these quanti- 
ties easily or accurately at this time, and we must accept them as nebulous 
concepts which are useful in establishing some background only. 

The physical device whose operation is based inherently on mutual 
inductance is the transformer. The 60-Hz power systems use many trans- 
formers, ranging in size from the dimensions of a living room to those of 
the living-room wastebasket. They are used to change the magnitude of 
the voltage, increasing it for more economical transmission, and then 
decreasing it for safer operation of home or industrial electrical equipment. 
Most radios contain one or more transformers, as do television receivers, 
hi-fi systems, some telephones, automobiles, and electrified railroads (Penn 
Central and Lionel both). 

We must next define mutual inductance and study the methods whereby 
its effects are included in the circuit equations. We shall conclude with 
a study of the important characteristics of a linear transformer and an 
important approximation to a good iron-core transformer which is known 
as an ideal transformer. 


When we defined inductance, we did so by specifying the relationship 
between the terminal voltage and current, 


We did learn, however, that the physical basis for such a current-voltage 
characteristic rests upon (1) the production of a magnetic flux by a current, 
the flux being proportional to the current in linear inductors; and (2) the 
production of a voltage by the time-varying magnetic field, the voltage 
being proportional to the time rate of change of the magnetic field or the 
magnetic flux. The proportionality between voltage and time rate of 
change of current thus becomes evident. 

Mutual inductance results from a slight extension of this same argument. 
A current flowing in one coil establishes a magnetic flux about that coil 
and also about a second coil which is in its vicinity; the time-varying flux 
surrounding the second coil produces a voltage across the terminals of this 
second coil; this voltage is proportional to the time rate of change of the 

433 Magnetically Coupled Circuits 

current flowing through the first coil. Figure 15-la shows a simple model 
of two coils Lj and L 2 sufficiently close together that the flux produced 
by a current i^t) flowing through L t establishes an open-circuit voltage 
v 2 (t) across the terminals of 1^. Without considering the proper algebraic 
sign for the relationship, we define the coefficient of mutual inductance, 
or simply mutual inductance M 21 , 

» 2 « = M 21 ^ (1) 

The order of the subscripts on M 21 indicates that a voltage response is 
produced at L 2 by a current source at L v If the system is reversed, as 
indicated in Fig. 15-lfe, and a voltage response is produced at Lj by a 
current source at L 2 , then we have 


«iW = M i2-Jr ( 2 ) 

Two coefficients of mutual inductance are not necessary, however; we shall 
use energy relationships a little later to prove that M 12 and M 21 are equal. 
Thus, M 12 = Af 21 = M. The existence of mutual coupling between two 
coils is indicated by a double-headed arrow, as shown in Fig. 15-la and b. 

Mutual inductance is measured in henrys and, like resistance, induc- 
tance, and capacitance, is always positive. 1 The voltage M di/dt, however, 
may appear as either a positive or a negative quantity in the same way 
that v = — Ri is useful. 

The inductor is a two-terminal element, and we are able to use the 
passive sign convention in order to select the correct sign for the voltage 
L di/dt, juLl, or sLI. If the current enters the terminal at which the positive 
voltage reference is located then the positive sign is used Mutual induc- 

Fig. 15-1 (a) A current ^ at Lj produces an open-circuit voltage v 2 at L 2 . 
[b) A current »2 at L 2 produces an open-circuit voltage v t at L v 



1 Mutual inductance is not universally assumed to be positive. It is particularly convenient 
to allow it to "cany its own sign" when three or more coils are involved and each coil 
interacts with each other coil. We shall restrict our attention to the more important simple 
case of two coils. 


= M 



c, = -M 



Fig. 1 5-2 Current entering the dotted terminal of one coil produces a voltage 
which is sensed positively at the dotted terminal of the second coil. Current 
entering the undotted terminal of one coil produces a voltage which is sensed 
positively at the undotted terminal of the second coil. 

tance, however, cannot be treated in exactly the same way because four 
terminals are involved. The choice of a correct sign is established by use 
of one of several possibilities which include the "dot convention," or an 
extension of the dot convention which involves the use of a larger variety 
of special symbols, or by" an examination of the particular way in which 
each coil is wound. We shall use the dot convention and merely look briefly 
at the physical construction of the coils; the use of other special symbols 
is not necessary when only two coils are coupled. 

The dot convention makes use of a large dot placed at one end of each 
of the two coils which are mutually coupled. A current entering the dotted 
terminal of one coil produces an open-circuit voltage between the terminals 
of the second coil which is sensed in the direction indicated by a positive 
voltage reference at the dotted terminal of this second coil. Thus, in Fig. 
15-2a, i x enters the dotted terminal of L x , v 2 is sensed positively at the 
dotted terminal of L 2 , and thus v 2 = M dijdt. We have found previously 
that it is often not possible to select voltages or currents throughout a circuit 
so that the passive sign convention is everywhere satisfied; the same situa- 
tion arises with mutual coupling. For example, it may be more convenient 
to represent v 2 by a positive voltage reference at the undotted terminal, 
as shown in Fig. 15-2&: then v 2 = — Mdijdt. Currents which enter the 
dotted terminal are also not always available, as indicated by Fig. 15-2c 
and d. Such a current provides a voltage which is positive at the undotted 
terminal of the second coil. 

We have as yet considered only a mutual voltage present across an 
open-circuited coil. In general, a nonzero current will be flowing in each 


Fig. 15-3 (a) Since the pairs v v i r and v 2 , i 2 each satisfy the passive sign 
convention, the voltages of self-induction are both positive; since i t and i 2 
each enter dotted terminals, and since v x and v 2 are both positively sensed 
at the dotted terminals, the voltages of mutual induction are also both positive. 
[b] Since the pairs t^, ij and v 2 , i 2 are not sensed according to the passive 
sign convention, the voltages of self-induction are both negative; since i x enters 
the dotted terminals and v 2 is positively sensed at the dotted terminal, the 
mutual term of v 2 is positive; and since i 2 enters the undotted terminal and 
v 1 is positively sensed at the undotted terminal, the mutual term of v t is also 

of the two coils, and a mutual voltage will be produced in each coil because 
of the current flowing in the other coil. This mutual voltage is present 
independently of any voltage of self-induction. In other words, the voltage 
across the terminals of L x will be composed of two terms L x dijdt and 
Mdi 2 /dt, each carrying a sign depending on the current directions, the 
assumed voltage sense, and the placement of the two dots. In the portion 
of a circuit drawn in Fig. 15-3a, currents i x and i 2 are shown, each arbitrarily 
assumed entering the dotted terminal. The voltage across L x is thus com- 
posed of two parts, 

d»i ^_ t/f di 2 

as is the voltage across L 2 , 

1 dt dt 

r di 2 , , dL 

L 2 — ± + M^- 

i dt dt 

In Fig. 15-3& the currents and voltages are not selected with the object 
of obtaining all positive terms for v x and v 2 . By inspecting only the 
reference symbols for i t and v t , it is apparent that the passive sign conven- 
tion is not satisfied and the sign of L x di x /dt must therefore be negative. 
An identical conclusion is reached for the term L 2 di 2 /dt. The mutual term 
of v 2 is signed by inspecting the direction of i t and v 2 ; since i x enters the 
dotted terminal and v 2 is positive at the dotted terminal, the sign of M dijdt 
must be positive. Finally, i 2 enters the undotted terminal of L 2 and v t is 
positive at the undotted terminal of L t ; hence, the mutual portion of v v 
M di 2 /dt, must also be positive. Thus, we have 


436 Two-port Networks 

di t 

-L^ + M^ 

di 2 

u, = -L. 

*2 + M f«l 



The same considerations lead to identical choices of signs for excitation 
at a complex frequency s, 

Vj = -sLjl! + sMI 2 

or at a real frequency s = /to, 

Vj = — /wLjIj + fuMl 2 

-;<oL 2 I 2 + /'wMIj 

Before we apply the dot convention to the analysis of a numerical 
example, we can gain a more complete understanding of the dot symbolism 
by looking at the physical basis for the convention. The meaning of the 
dots is now interpreted in terms of magnetic flux. Two coils are shown 
wound on a cylindrical form in Fig. 15-4, and the direction of each winding 
is evident. Let us assume that the current i t is positive and increasing with 
time. The magnetic flux that i t produces within the form has a direction 
which may be found by the right-hand rule: when the right hand is wrapped 
around the coil with the fingers pointing in the direction of current flow, 
the thumb indicates the direction of the flux within the coil. Thus i t 
produces a flux which is directed downward; since i x is increasing with 
time, the flux, which is proportional to i v is also increasing with time. 
Turning now to the second coil, let us also think of i 2 as positive and 
increasing; the application of the right-hand rule shows that i 2 also produces 
a magnetic flux which is directed downward and is increasing. In other 
words, the assumed currents i t and i 2 produce additive fluxes. 

Fig. 15-4 The physical construction of two mutually coupled coils. From a 
consideration of the direction of magnetic flux produced by each coil, it is 
shown that dots may be placed either on the upper terminal of each coil or 
on the lower terminal of each coil. 

M = 9H 

-^ l H 

O) = 10 rad/s 

Fig. 1 5-5 A circuit containing mutual inductance in which the voltage ratio 
V 2 /V x is desired. 

The voltage across the terminals of any coil results from the time rate 
of change of the flux linking that coil. The voltage across the terminals 
of the first coil is therefore greater with i 2 flowing than it would be if i 2 
were zero. Thus i 2 induces a voltage in the first coil which has the same 
sense as the self-induced voltage in that coil. The sign of the self-induced 
voltage is known from the passive sign convention, and the sign of the 
mutual voltage is thus obtained. 

The dot convention merely enables us to suppress the physical con- 
struction of the coils by placing a dot at one terminal of each coil such 
that currents entering dot-marked terminals produce additive fluxes. It is 
apparent that there are always two possible locations for the dots, because 
both dots may always be moved to the other ends of the coils and additive 
fluxes will still result. 

The alternative method of selecting the correct signs for the mutual 
terms therefore consists of first noting whether or not both currents enter 
dot-marked terminals. If they do, then the sign of the mutual voltage at 
each coil is the same as the sign of the self-induced voltage at that same 
coil. The same result occurs if both currents leave dot-marked terminals. 
However, if neither of these conditions occurs, then subtractive fluxes result 
and the sign of the mutual voltage at each coil is the opposite of the sign 
of the self-induced voltage at that same coil. 

In the example of Fig. 15-3fo, the currents do not both enter either the 
dotted or undotted terminals, and the signs of the mutual terms must be 
the opposite of the signs of the self-induced terms. The passive sign 
convention indicates that both of the self-induced voltages carry negative 
signs, and thus both of the mutual voltages are positive. This agrees with 
the previous set of equations obtained for this circuit; either method may 
be used to find the correct signs for the M di/dt terms. 

Let us now apply these methods to the analysis of the circuit outlined 
in Fig. 15-5. We desire the ratio of the output voltage across the 400-fi 
resistor to the source voltage. Two conventional mesh currents are estab- 
lished, and Kirchhoff's voltage law must next be applied to each mesh. 
In the left mesh, the sign of the mutual term may be determined, for 
example, by applying the dot convention directly. Since I 2 leaves the 
dot-marked terminal of Lg, the mutual voltage across L x must have the 
positive reference at the undotted terminal. Thus, 


438 Two-port Networks 

1^1 + /10) - /90I 2 = 10 

For variety, the sign of the mutual term in the second mesh may be 
determined by another method. Since Ij enters the dot-marked terminal 
while I 2 leaves the dot-marked terminal, the mutual term in each mesh 
must have the opposite sign from the self-inductance term. Thus, we may 

I 2 (400 + /1000) - f901 t = 

The two equations may be solved by determinants (or a simple elimination 

of LJ, 

| 1 + /10 10 I 

I -;90 I 

1 + ;10 -;90 I 

-/90 400 + /1000 I 

T„ = 0.1725/ -16.7° 

and thus 

V 2 400(0.1725/ -16.7°) 
Vj _ 10 


^2. = 6.90/- 16.7° 

The output voltage is greater in magnitude than the input voltage, and 
thus a voltage gain is possible with mutual coupling just as it is in a resonant 
circuit. The voltage gain available in this circuit, however, is present over 
a relatively wide range of frequency; in a moderately high Q resonant 
circuit, the voltage step-up is proportional to the Q and occurs only over 
a range of frequency which is inversely proportional to Q. Let us see if 
this point can be made clear by reference to the complex plane. 

We may find I 2 (s) for this particular circuit, 

II + s VJ 
I M I -9s I _ 9sV 1 

l 2( s > - , 1 + s _ 9s | 19s 2 + 500s + 400 

I -9s 400 + 100s I 
and thus obtain the ratio of output to input voltage as a function of s, 

V 2 3600s _ 

V, ~ 19s 2 + 500s + 400 ' (s -I- 0.826)(s + 25.5) 




Fig. 1 5-6 A pole-zero plot of the transfer function Vj/Vj for the circuit shown 
in Fig. J 5-5. The plot is useful in showing that the magnitude of the transfer 
function is relatively large from to = 1 or 2 to to = 1 5 or 20. 

The pole-zero plot of this transfer function is shown in Fig. 15-6. The 
location of the pole at s = —25.5 is distorted in order to show both poles 
clearly; the ratio of the distances of the two poles from the origin is actually 
about 30:1. An inspection of this plot shows that the transfer function 
is zero at zero frequency but that as soon as to is greater than, say, 1 or 
2 the ratio of the distances from the zero and the pole nearer the origin 
is essentially unity. Thus the voltage gain is affected only by the distant 
pole on the negative a axis, and this distance does not increase appreciably 
until to approaches 15 or 20. 

These tentative conclusions are verified by the response curve of Fig. 
15-7, which shows that the magnitude of the voltage gain is greater than 
0.707 of its maximum value from to = 0.78 to <o = 26. 

The circuit is still passive, except for the voltage source, and the voltage 
gain must not be mistakenly interpreted as a power gain. At to = 10, the 

Fig. 1 5-7 The voltage gain | V 2 /Vj| of the circuit shown in Fig. 1 5-5 is plotted 
as a function of w. The voltage gain is greater than 5 from about a = 0.75 
to approximately w = 28. 



Fig. 15-8 A three-mesh circuit with mutual coupling may be analyzed most 
easily by loop or mesh methods. 

voltage gain is 6.90, but the ideal voltage source, possessing a voltage of 
10 V, delivers a total power of 8.08 W of which only 5.95 W reaches the 
400-fi resistor. The ratio of the output power to the source power, which 
we may define as the power gain, is thus 0.737. 

Let us consider briefly one additional example, illustrated in Fig. 15-8. 
The circuit contains three meshes, and three mesh currents are assigned. 
Applying Kirchhoff's voltage law to the first mesh, a positive sign for the 
mutual term is assured by selecting (I 3 — I 2 ) as the current through the 
second coil. Thus, 

5Ii + 78(1! - I 2 ) + 2s(I 3 - I 2 ) = V x 
(5 + 7s)l! - 9sl 2 + 2sl 3 = Vj 


The second mesh requires two self-inductance terms and two mu- 
tual-inductance terms; the equation cannot be written carelessly. We obtain 

7s(I 2 - I x ) + 2s(I 2 - I 3 ) + -i-I 2 + 6s(I 2 - I 3 ) + 2s(I 2 - I,) = 

-9SIJ + (l7s + 1) I 2 - 8sl 3 = (4) 


Finally, for the third mesh 

6s(I 3 - Ijj) + 2s(Ij - I 2 ) + 3I 3 = 
2sl x - 8sl 2 + (3 + 6s)I 3 = 


Equations (3) to (5) may be solved by any of the conventional methods. 

Drill Problems 

1 5-1 Refer to the coupled coils shown in Fig. 15-3o and let Lj =4H,I 2 = 3H, 
and M = 2 H. Find v 2 if: (a) i x = 5 cos 6* A, i 2 = 0; (b) i t = 0, i 2 = 3 cos 6t A; 
(c) »! = 5 cos 6f, i 2 = 3 cos 6t A. 

Ans. -114 sin 6t; -60sin6t; -54sin6t V 


44 1 Magnetically Coupled Circuits 

1 5-2 In the circuit shown in Fig. 15-9, find: (a) I 2 ; (b) I x ; (c) 1 R . 

Ans. 17,9 / -153.4° ; 1.79 /26.6° ; 2.53 / -18.4° mA 

4 cos 5000 / (fy 

Fig. 15-9 See Drill Probs. 15-2 and 15-3. 

1 5-3 For the circuit of Fig. 15-9, let the current source be I 8 and the voltage 
across the 5-52 resistor (positive reference up) be V 2 . Find V 2 /I 5 as a function 
of s and evaluate for s = : (a) -2000; (b) /5000; (c) -2500 + /5000 s" 1 . 

Ans. 22.4 /26.6° ; 27.9 /26.6° ; -100 U 


Let us now consider the energy stored in a pair of mutually coupled 
inductors. The results will be useful in several different ways. We shall 
first justify our assumption that M 12 — M 2V and we may then determine 
the maximum possible value of the mutual inductance between two given 
inductors. Finally, we shall provide ourselves with a basis from which it 
is possible to establish the initial conditions in magnetically coupled circuits, 
although we shall consider only the more elementary cases. 

A pair of coupled coils is shown in Fig. 15-3a with currents, voltages, 
and polarity dots indicated. Let us first show that reciprocity is valid, or 
that M 12 = M 21 . In order to do so, we shall begin by letting all currents 
and voltages be zero, thus establishing zero initial energy storage in the 
network. We first open-circuit the right terminal pair and increase i x from 
zero to some constant value I v The power entering the network from the 
left at any instant is 

and that entering from the right is 

since i 2 = 0. 

The energy stored within the network when tj = I x is thus 

442 Tw °-P° rt Networks 

Djij dt = I Ljij di x = 1 / 2 L 1 I 1 2 
u J o 

We now hold i x constant, i x = I 1 , and let i 2 change from zero to some 
constant value I 2 . The energy delivered from the right source is thus 

J*2 ~*2 

v 2 i 2 dt = I L 2 i 2 di 2 = Y 2 L 2 I 2 2 
11 J o 

However, even though the value of i x remains constant, the left source 
also delivers energy to the network during this time interval, 

X t2 r t2 di 

v 1 i 1 dt = j M 12 -^-i 1 dt 

c' 2 

= M 12 l x I di 2 

M 12 hl 


The total energy stored in the network when both i x and i 2 have reached 
a constant value is 

w^ = y^'i 2 + y 2 v 2 2 + mm 

Now we may establish the same final currents in this network by 
allowing the currents to reach their final values in the reverse order, that 
is, first increasing i 2 from zero to I 2 and then holding i 2 constant while 
«j increases from zero to I x . If the total energy stored is calculated for 
this experiment, the result is found to be 

w totaJ = y 2 w 2 + %l 2 i 2 2 + M 21 y 2 

The only difference is the interchange of the mutual inductances M 21 and 
M 12 . The initial and final conditions in the network are the same, however, 
and the two values of the stored energy must be identical. Thus, 

M 12 = M 21 = M 
and W = YJLJ, 2 + x / 2 L 2 l 2 + M hh ( 6 ) 

If one current enters a dot-marked terminal while the other leaves a 
dot-marked terminal, the sign of the mutual energy term is reversed: 

W = yjsj* + %£,/,* - MI,I 2 (7) 

443 Magnetically Coupled Circuits 

Although (6) and (7) were derived by treating the final values of the 
two currents as constants, it is apparent that these "constants" may have 
any value, and the energy expressions correctly represent the energy stored 
when the instantaneous values of i t and i 2 are /j and J 2 , respectively. In 
other words, lowercase symbols might just as well be used, 

w{t) = y^Mtf? + 1 /W 2 «] 2 ± WMWi\ (8) 

The only assumption upon which (8) is based is the logical establishment 
of a zero-energy reference level when both currents are zero. 

Equation (8) may now be used to establish an upper limit for the value 
of M. Since w(t) represents the energy stored within a passive network, 
it cannot be negative for any values of i v i 2 , L v L 2 , or M. Let us assume 
first that i x and i 2 are either both positive or both negative; their product 
is therefore positive. From (8), the only case in which the energy could 
possibly be negative is 

W = 1 /2 J Vl Z + y2 L 2»2 2 - Mi lh 

which we may write, by completing the square, 

«j = y 2 ( VL[h - V^i 2 ) 2 + ^fW^HH - Mi ih 

Now the energy cannot be negative; the right side of this equation therefore 
cannot be negative. The first term, however, may be as small as zero, and 
thus the sum of the last two terms cannot be negative. Hence, 


There is, therefore, an upper limit to the possible magnitude of the 
mutual inductance; it can be no larger than the geometric mean of the 
inductances of the two coils between which the mutual inductance exists. 
Although we have derived this inequality on the assumption that »j and 
i 2 carried the same algebraic sign, a similar development is possible if the 
signs are opposite; it is only necessary to select the positive sign in (8). 

We might also have demonstrated the truth of (9) from a physical 
consideration of the magnetic coupling; if we think of i 2 as being zero and 
the current i 1 as establishing the magnetic flux linking both L x and L 2 , it 
is apparent that the flux linking L 2 cannot be greater than the flux linking 
L x , which represents the total flux. Qualitatively, then, there is an upper 
limit to the magnitude of the mutual inductance possible between two given 
inductors. For example, if L x — 1 H and L 2 = 10 H, then M < 3.16 H. 

444 Two-port Networks 

The degree to which M approaches its maximum value is exactly 
described by the coefficient of coupling. We define the coefficient of 
coupling, symbolized as k, 



It is evident that 

< * < 1 

The larger values of the coefficient of coupling are obtained with coils 
which are physically closer, which are wound or oriented to provide a larger 
common magnetic flux, or which are provided with a common path through 
a material which serves to concentrate and localize the magnetic flux (a 
high-permeability material). Coils having a large coefficient of coupling 
are said to be tightly coupled. 

The complete response of a circuit possessing mutual coupling must 
of course be made up of the sum of a forced and a natural response. We 
are now equipped to find the forced response for the more familiar forcing 
functions, and we shall consider this portion of the response in detail for 
several interesting circuits in the remainder of this chapter. If we can find 
the forced response, then we certainly can locate the poles or zeros of any 
immittance function associated with the circuit. This knowledge of the 
pole-zero locations then enables us to establish the functional form of the 
natural response. The remaining problem, the determination of the arbi- 
trary constants through the values of the initial conditions in the network, 
is not as easily resolved with the analytical methods we possess. The use 
of the initial conditions turns out to be much more straightforward when 
the operational method of the Laplace transform is employed, and this topic 
is one which we shall investigate in Chap. 19. Rather than make a simple 
problem appear difficult, we shall therefore largely neglect the transient 
analysis of mutually coupled circuits at this time. Let us consider only 
the single straightforward problem of finding the complete response when 
a constant voltage is suddenly applied to one coil while the second coil 
is connected to a resistive load. 

The circuit to be analyzed is shown in Fig. 15-10; the currents i t and 
i 2 are desired. The forced response may be determined readily, for it will 
have the form of the forcing function, that is, a constant times u(t). Since 
neither current is changing, there can be no mutual voltage. Thus, i 2 is 
flowing in a source-free circuit and this forced response must be zero. The 
10-V source present in the first mesh, however, produces a forced response 
of 5 A for i r Thus, 

io u(t) vVi 

Fig. 15-10 A circuit containing mutual inductance for which the complete 
response is desired. 

i lf = 5u(t) i 2f = 

The form of the natural response is now obtained by determining the 
zeros of the impedance offered to the source. After writing the Kirchhoff 
voltage equation about each mesh, 

(2 + 2.5s)!! + 2sl 2 = \ 1 
2sl x + (8 + 4s)I 2 = 

we determine Z, n as the ratio of Vj to I v 

4s 2 

Z, n = 2 + 2.5s ■ 

8 + 4s 

Z, = Lst' + W'-M 
^ n s + 2 

and thus the form of the natural response is established for both i x and « 2 , 

« lB = A ie - 2t/3 + B ie - 4 * 
i 2n = A 2 e~ 2l/3 + B 2 e-« 

The complete responses are therefore 

ij = 5u(t) + A ie - 2,/3 + B ie - 4 ' (11) 

i 2 = A 2 e-*"3 + B 2 e-« (12) 

We must next establish the initial values of the two currents and their 
first derivatives from physical considerations. There is no energy stored 
initially in the circuit, and there can be no discontinuous change in the 
stored energy without the presence of an impulse source. Thus, the energy 
stored remains zero at t — + , and this requires that both i x and i 2 be zero 
at t = + . The initial values of the two derivatives are most easily found 
by using the time-domain statements of Kirchhoff 's voltage law for each 


446 Two-pert Networks 

2i t + 2.5 -^ + 2^ = 10u(t) 

At £ = + , we have 

2 *1 

+ 8i 2 

, di, 

+ 4 dF = 


+ 2.5 

di x 1 
df 1 * 

~<^*2 1 


= 10 

9 *i| 
dt I 

. din 1 
0* <« 1 



Solving simultaneously, 

di l I - — A *1 I 10 

dt I 0+ 3 dt I 0+ 3 

Taking the derivative of (11) and (12) and evaluating at t = + , we therefore 



1 = ^ = _^_ 4Bl 

l ot 3 3 

di 2 

1 = W _^_4B 2 
L 3 3 2 

Since each current is also initially zero, 

Aj + B t + 5 = A 2 + B 2 = 

These last four equations may be solved easily for the four arbitrary 
constants. When the results are inserted in (11) and (12), we obtain 

t! = 5 - 4e~ 2t/3 - e~ 4 ' 
i 2 = -e- 2t/3 + e~ 4t 

for t > 0. 

The source current is quite similar to the response of the simple RL 
series circuit having a time constant of approximately 4 s. The value of 
4 s, however, is determined by both resistors, both self-inductances, and 
the mutual inductance. The load current is a negative pulse having a 
maximum magnitude of about 0.6 A, occurring about 0.5 s after t = 0. 

The principles on which this analysis is based are not difficult to com- 
prehend, but one does suffer from fatigue in carrying out the analytical 

447 Magneticolly Coupled Circuits 

details. The use of operational methods serves to reduce greatly the number 
of trivial steps required, as well as to organize the solution in a more 
systematic fashion. 

Drill Problems 

1 5-4 If currents tj and i 2 enter the dotted terminals of a pair of coupled coils, 
Lj = 0.2 H, L 2 = 1.25 H, k = 0.8, find the total energy stored in the system at 

t = if: (a) ij = i 2 = 4 cos u>t A; (b) i 1 = — i 2 — 4 cos oit A; (c) i 1 = 2e~" f , ij = 
2 cos <ot A. 

Ans. 4.5; 5.2; 18 J 

1 5-5 In the circuit shown in Fig. 15-10, change M to 0.8 H and find the initial 
values (t = 0+) of: (a) » i; (b) dijdt; (c) (P^/dt 2 . 

Ans. -4.24 A/s 2 ; 0; 4.27 A/s 

1 5-6 Two inductors, L t = 25L 2 = 1 H, are mutually coupled with k = 1. An 
impedance Z L is connected across L 2 . Find the input impedance at the terminals 
of L x at w = 1000 rad/s if Z L = : (a) 4; lb) j4; (c) -j4 SI. 

Ans. -jlll.l; J90.9; 99.0 + J9.90 Q 


We are now ready to apply our knowledge of magnetic coupling to an 
analytical description of the performance of two specific practical devices, 
each of which may be represented by a model containing mutual induc- 
tance. Both of the devices are transformers, a term which we may define 
as a network containing two or more coils which are deliberately coupled 
magnetically. In this section we shall consider the linear transformer, which 
is, even in practice, a linear device finding its greatest application at radio 
frequencies, or higher frequencies. In the following section we shall con- 
sider the ideal transformer, which is an idealized unity-coupled model of 
a physical transformer that has a core made of some magnetic material, 
usually iron alloy. 

In Fig. 15-11 there is shown a transformer with two mesh currents 
identified. The first mesh, usually containing the source, is called the 
primary, while the second mesh, usually containing the load, is known as 
the secondary. The inductors L x and L 2 are also referred to as the primary 
and secondary, respectively, of the transformer. We shall assume that the 
transformer is linear. This merely infers that no magnetic material is 
employed to cause most of the magnetic flux produced by the primary 
winding to link the secondary winding. Without such material, it is difficult 

Fig. 15-11 A linear transformer containing a source in the primary circuit 
and a load in the secondary circuit. Resistance is also included in both the 
primary and secondary. 

to achieve a coefficient of coupling greater than a few tenths. The two 
resistors serve to account for the resistance of the wire out of which the 
primary and secondary coils are wound, and any other losses. 

In many applications, the linear transformer is used with a tuned, or 
resonant, secondary; the primary winding is also operated often in a 
resonant condition by replacing the ideal voltage source by a current source 
in parallel with a large resistance and a capacitance. The analysis of such 
a single-tuned or double-tuned circuit is a fairly lengthy process, and we 
shall not undertake it at this time. It may be pointed out, however, that 
the secondary response is characterized by the familiar resonance curve 
for relatively small coefficients of coupling but that a greater control of 
the shape of the response curve as a function of frequency becomes possible 
for larger coefficients of coupling. Response curves which possess flatter 
tops and sharper drops on each side may be achieved in the double-tuned 

Let us consider only the input impedance offered at the terminals of 
the primary circuit. The two mesh equations are 

V s = I 1 (fl 1 + dj - I 2 sM (13) 

= -I lS M + I 2 (R 2 + sL 2 + Z L ) (14) 

We may simplify by defining 

Z ll = R l + SL 1 Z 22 = fi 2 + SL 2 + Z L 

and thus 

V, = I,Z n - I 2 sM (15) 

= -IjsM + I 2 Z 22 (16) 

Solving the second equation for I 2 and inserting this in the first equation 
enables us to find the input impedance, 

V s 2 M 2 

Zin = ^ = Z« - '-f- (17) 

*1 ^22 


449 Ma sn*ti«>lly Coupled Circuits 

Before manipulating this expression any further, we can draw several 
exciting conclusions. In the first place, this result is independent of the 
location of the dots on either winding, for if either dot is moved to the 
other end of the coil, the result is a change in sign of each term involving 
M in (13) to (16). This same effect could be obtained by replacing M by 
(— M), and such a change cannot affect the input impedance, as (17) 
demonstrates. We also may note in (17) that the input impedance is simply 
Z n if the coupling is reduced to zero. As the coupling is increased from 
zero, the input impedance differs from Z u by an amount — s 2 M 2 /Z 22 , termed 
the reflected impedance. This change can be inspected more closely by 
letting s = ;'co, 

Zin(/ W ) = Z ll(/<°) + • 

and rationalizing the reflected impedance, 

Z,n = Zu + 

u 2 M 2 R 22 _ -p 2 M 2 X 2 . 

11 R 2 ■ V 2^R 2 j y 2 

"22 I A 22 "22 ^ A 29 

22 ~ A 22 

Since u> 2 M 2 R 22 /(R 2 2 2 + -^22 2 ) mus t be positive, it is evident that the pres- 
ence of the secondary increases the losses in the primary circuit. In other 
words, the presence of the secondary might be accounted for in the primary 
circuit by increasing the value of R v Moreover, the reactance which the 
secondary reflects into the primary circuit has a sign which is opposite to 
that of X 22 , the net reactance around the secondary loop. This reactance 
X 22 is the sum of uiL, and X L ; it is necessarily positive for inductive loads 
and either positive or negative for capacitive loads, depending on the 
magnitude of the load reactance. 

Let us consider the effects of this reflected reactance and resistance 
by considering the special case in which both the primary and secondary 
are identical series-resonant circuits. Thus, R t — R 2 .— R, L-^ — l^ — L, 
and the load impedance Z L is produced by a capacitance C, identical to 
a capacitance inserted in series in the primary circuit. The series-resonant 
frequency of either the primary or secondary alone is thus to = 1/ -\/LC. 
At this resonant frequency, the net secondary reactance is zero, the net 
primary reactance is zero, and no reactance is reflected into the primary 
by the secondary. The input impedance is therefore a pure resistance; a 
resonant condition is present. At a slightly higher frequency, the net 
primary and secondary reactances are both inductive, and the reflected 
reactance is therefore capacitive. If the magnetic coupling is sufficiently 
large, the input impedance may once again be a pure resistance; another 
resonant condition is achieved, but at a frequency slightly higher than <o . 
A similar condition will also occur at a frequency slightly below w . Each 
circuit alone is capacitive, the reflected reactance is inductive, and cancel- 
lation may occur. 

450 Two-port Networks 

Although we are leaping at conclusions, it seems possible that these 
three adjacent resonances, each similar to a series resonance, may permit 
a relatively large primary current to flow from the voltage source. The 
large primary current in turn provides a large induced voltage in the 
secondary circuit, and a large secondary current. The secondary current 
is present over a band of frequencies extending from slightly below to 
slightly above <o , and thus a maximum response is achieved over a wider 
range of frequencies than is possible in a simple resonant circuit. Such 
a response curve is obviously desirable if the primary source is some 
intelligence signal containing energy distributed throughout a band of 
frequencies, rather than at a single frequency. Such signals are present 
in AM and FM radio, television, telemetry, radar, and all other communi- 
cation systems. 

It is often convenient to replace a transformer by an equivalent network 
in the form of a T or it. If we separate the primary and secondary resist- 
ances from the transformer, only the pair of mutually coupled inductors 
remains, as shown in Fig. 15-12. The differential equations describing this 
circuit are, once again, 

dt + 2 dt 

and v 2 = M-± + L 2 ^ (19) 

The form of these two equations is familiar and may be easily interpreted 
in terms of mesh analysis. Let us select a clockwise i t and a counterclock- 
wise i 2 so that ij and i 2 are exactly identifiable with the currents in Fig. 
15-12. The terms Mdi 2 /dt in (18) and Mdijdt in (19) indicate that the 
two meshes must then have a common seZ/-inductance M. Since the total 
inductance around the left mesh is L v a self-inductance of L x — M must 
be inserted in the first mesh, but not in the second mesh. Similarly, a 
self-inductance of L 2 — M is required in the second mesh, but not in the 
first mesh. The resultant equivalent network is shown in Fig. 15-13. The 
equivalence is guaranteed by the identical pairs of equations relating v v 
i ly v 2 , and i 2 for the two networks. 

Fig. 15-12 A given transformer which may be replaced by the equivalent 
networks shown either in Fig. 15-13 or 15-14. 


-onnp 1 'otip- 


Fig. 15-13 The T equivalent of the transformer shown in Fig. 15-12. 

If either of the dots on the windings of the given transformer is placed 
on the opposite end of its coil, the sign of the mutual terms in (18) and 
(19) will be negative. This is analogous to replacing M by — M, and such 
a replacement in the network of Fig. 15-13 leads to the correct equivalent 
for this case. 

The inductances in the T equivalent are all self-inductances; no mutual 
inductance is present. It is possible that negative values of inductance may 
be obtained for the equivalent circuit, but this is immaterial if our only 
desire is a mathematical analysis; the actual construction of the equivalent 
network is of course impossible in any form involving a negative inductance. 

The equivalent 77 network is not obtained as easily; it is more compli- 
cated, and it is not used as much. We develop it by solving (19) for di 2 /dt 
and substituting the result into (18), 

di x M M 2 di x 

°i = L ^ + 

-v~ - ■ 

dt ' h, " 2 L, dt 

i^ 2 

° r dF = L,L 2 - M 2 Vl ~ L,L 2 - M 2 V2 

If we now integrate from to t, we obtain 

L r* Mr' 

<i - ^ (0) " (f) = Z,L 2 -M 2 4, V > dt - ^-W l °* dt 

In a similar fashion, we also have 



Equations (20) and (21) may be interpreted as a pair of nodal equations. 
A step-current source must be installed at each node in order to provide 
the proper initial conditions. The factors multiplying each integral are 
evidently the inverses of certain equivalent inductances. Thus, the second 
coefficient in (20), M/(L X L 2 - M 2 ), is 1/L B> or the reciprocal of the in- 
ductance extending between nodes 1 and 2, as shown on the equivalent 


i,(0)u(*) T 2 r 

^fc? * 


Fig. 15-14 The tt network which is equivalent to the transformer shown 
Fig. 15-12. 

it network, Fig. 15-14. The first coefficient in (20), 1^/(1^1^ - M 2 ), is 
l/L A + l/L B . Thus, 


J__ L 2 

L A ~ L^L 2 - M 2 ~ L t L 2 - M 2 

. _L 1 L 2 -M 2 


L r .= 

L t L 2 - M 2 
L, - M 

No magnetic coupling is present among the inductances in the equivalent 
circuit, and the initial currents in the three self-inductances are zero. 

We may compensate for a reversal of either dot in the given transformer 
by merely changing the sign of M in the equivalent network. Also, just 
as we found in the equivalent T, negative self-inductances may appear in 
the equivalent network. 

Drill Problems 

1 5-7 Find the three inductances appearing in the T equivalent of the transformer 
shown in Fig. 15-15 if L 2 = 4 H, and the input inductance at A-B is 6 H with 
C-D open-circuited and 2 H with C-D short-circuited. 

Ans. -4; 8; 10 H 

Fig. 15-15 See Drill Probs. 15-7 to 15-9. 



'■» {.* 


453 Magnetically Couplvd Circuiti 

15-8 Find the three inductances appearing in the -n equivalent of the transformer 
shown in Fig. 15-15 if i t = 2 mH, L 2 = 8 mH, and k = 0.1. 

Ans. -39.6; 1.89; 6.60 mH 

15-9 Let Lj = 0.1 H, Lj = 0.4 H, and M = 0.12 H in the transformer of Fig. 
15-15. Find the input inductance at terminals A-B if: (a) C is connected to D; 
(b) C is connected to A and D to B; (c) C is connected to B and D to A. 

Ans. 34.6; 64.0; 98.5 mH 


An ideal transformer is a useful approximation of a very tightly coupled 
transformer in which the coefficient of coupling is almost unity and both 
the primary and secondary inductive reactances are extremely large in 
comparison with the terminating impedances. These characteristics are 
closely approached by most well-designed iron-core transformers over a 
reasonable range of frequencies for a reasonable range of terminal im- 
pedances. The approximate analysis of a circuit containing an iron-core 
transformer may be achieved very simply by replacing that transformer 
by an ideal transformer; the ideal transformer may be thought of as a 
first-order model of an iron-core transformer. 

One new concept arises with the ideal transformer, the turns ratio a. 
The self-inductance of either the primary or secondary coil is proportional 
to the square of the number of turns of wire forming the coil. This rela- 
tionship is valid only if all the flux established by the current flowing in 
the coil links all the turns. In order to develop this result logically, it is 
necessary to utilize magnetic-field concepts, a subject which is not included 
in our discussion of circuit analysis. However, a qualitative argument may 
suffice. If a current I flows through a coil of N turns, then N times the 
magnetic flux of a single-turn coil will be produced. If we think of the 
N turns as being coincident, then all the flux certainly links all the turns. 
As the current and flux change with time, a voltage is then induced in 
each turn which is N times larger than that caused by a single-turn coil. 
Finally, the voltage induced in the N-tum coil must be N 2 times the 
single-turn voltage. Thus, the proportionality between inductance and the 
square of the number of turns arises. It follows that 



a = — - 

7V 2 

Iv 2 2 



k - 1 

Fig. 15-16 An ideal transformer driven by a practical voltage source is 
connected to a general load impedance. 

Figure 15-16 shows an ideal transformer to which a secondary load and 
a primary source, including a source impedance, are connected. The ideal 
nature of the transformer is established by several conventions, the use of 
the vertical lines between the two coils to indicate the iron laminations 
present in many iron-core transformers, the unity value of the coupling 
coefficient, and the presence of the symbol 1 : a, suggesting a turns ratio 
of N t to N 2 . 

Let us analyze this transformer in the sinusoidal steady state in order 
that we may interpret our assumptions in the simplest context. The two 
mesh equations are 

V s = ^(Z, + i"L x ) - I 2 /<oM 
= — IrfaM + I 2 (Z L + juL. 



We first determine the input impedance of an ideal transformer. Although 
we shall let the self-inductance of each winding become infinite, the input 
impedance will remain finite. By solving (23) for I 2 and substituting into 
(22), we obtain 


V s = I 1 (Z + juLJ + h 

<0 2 M 2 

Z L + juL 2 
u 2 M 2 

Z £ + P L 2 

Since k = 1, M 2 = L t L 2 , and 

Zin = Z 5 + i"Ll + 

Z L + juL 2 

We now must let both L x and L 2 tend to infinity. Their ratio, however, 
remains finite, as specified by the turns ratio. Thus, 


455 Magiwtieolly Coupled Circuits 

L 2 = a 2 L-y 
and Z, n = Z g + F Z, + ^ + ^ 

Now if we let 1^ become infinite, both of the last two terms in the above 
expression become infinite, and the result is indeterminate. It is necessary 
to first combine these two terms, 

, \u>L^L h - ofia 2 h? + nVV . 

z * = z » + z^TJ^l, (24) 

Zin = Z, + • 

/toL 1 Z L 

» ^ Z t + foa% (25) 

Now as Lj becomes infinite, it is apparent that Zj n becomes 

** = *. + % < 26 > 

for finite Z L . 

This result has some interesting implications, and at least one of them 
appears to contradict one of the characteristics of the linear transformer. 
It should not, of course, since the linear transformer represents the more 
general case. The input impedance of the ideal transformer is the series ' 
combination of the generator impedance and an impedance which is 
proportional to the load impedance, the proportionality constant being the 
reciprocal of the square of the turns ratio. In other words, if the load 
impedance is a capacitive impedance, then the input impedance is the 
generator impedance plus a capacitive impedance. In the linear trans- 
former, however, the reflected impedance suffered a sign change in its 
reactive part; a capacitive load led to an inductive contribution to the input 
impedance. The explanation of this occurrence is achieved by first realizing 
that Z L /a 2 is not the reflected impedance, although it is often loosely called 
by that name. The true reflected impedance is infinite in the ideal trans- 
former; otherwise it could not "cancel" the infinite impedance of the 
primary inductance. This cancellation occurs in the numerator of the 
fraction in (24). The impedance Z L /a 2 represents a small term which is 
the amount by which an exact cancellation does not occur. The true 
reflected impedance in the ideal transformer does change sign in its reactive 
part; as the primary and secondary inductances become infinite, however, 
the effect of the infinite primary-coil reactance and the infinite, but nega- 
tive, reflected reactance of the secondary coil is one of cancellation. 

The first important characteristic of the ideal transformer is therefore 
its capability to change the magnitude of an impedance, or to change 

456 Two-port Networks 

impedance level. An ideal transformer having 100 primary turns and 10,000 
secondary turns has a turns ratio of 10,000/100, or 100. Any impedance 
placed across the secondary then appears at the primary terminals reduced 
in magnitude by a factor of 1O0 2 , or 10,000. A 20,000-0 resistor looks like 
2 0, a 200-mH inductor looks like 20 fiH, and a 100-pF capacitor looks 
like 1 jnF. If the primary and secondary windings are interchanged, then 
a = 0.01 and the load impedance is apparently increased in magnitude. 
In practice, this exact change in magnitude does not always occur, for we 
must remember that as we took the last step in our derivation and allowed 
Lj to become infinite in (25), it was necessary to neglect Z L in comparison 
with jo>L 2 . Since L 2 can never be infinite, it is evident that the ideal 
transformer model will begin to fail for large load impedances. 

A practical example of the use of an iron-core transformer as an 
impedance-level changing device is in the output of an audio power 
amplifier which must be connected to a loudspeaker. In order to achieve 
maximum power transfer, we know that the resistance of the load should 
be equal to the internal resistance of the source; the speaker usually has 
an impedance magnitude (often assumed to be a resistance) of only a few 
ohms, while the power amplifier possesses an internal resistance of several 
thousand ohms. An ideal transformer in which N 2 < N x is called for. For 
example, if the amplifier internal impedance is 4000 Q and the loudspeaker 
impedance is 8 Q, then we desire that 

Z g = 4000 = % = -i 

or a = — 5— 


and thus 

^ = 22.4 

There is also a simple relationship between the primary and secondary 
currents Ij and I 2 in an ideal transformer. From (23) 





+ Fi-2 


i allow L 2 

to become infinite, 

J 2 _ 




jaL 2 



r 2_ 



457 Mofl'ofaally Coupled Circuits 

The ratio of the primary and secondary currents is the turns ratio. If we 
have iV 2 > N v then a > 1, and it is apparent that the larger current flows 
in the winding with the fewer number of turns. In other words, 

N^ = N 2 I 2 

It should also be noted that the current ratio is the negative of the turns 
ratio if either current is reversed or if either dot location is changed. In 
the example above in which an ideal transformer was used to change the 
impedance level to match a loudspeaker efficiently to a power amplifier, 
an rms current of 50 mA at 1000 Hz in the primary causes an rms current 
of 1.12 A at 1000 Hz in the secondary. The power delivered to the 
loudspeaker is 1.12 2 (8), or 10 W, and the power delivered to the transformer 
by the power amplifier is (0.05) 2 4000, or 10 W. The result is comforting, 
since the ideal transformer does not contain either an active device which 
can deliver power or any resistance to absorb power. 

Since the power delivered to the ideal transformer is identical with 
that delivered to the load, whereas the primary and secondary currents 
are related by the turns ratio, it is obvious that the primary and secondary 
voltages must also be related to the turns ratio. If we define the secondary 
voltage, or load voltage, 

and the primary voltage as the voltage across L v then 

\ = Ix(Z,» - z; = hh 

The ratio of the two voltages is 

V, 1 

a ■■ 

V t Wi 


The ratio of the secondary to primary voltage is equal to the turns ratio. 
This ratio may also be negative if either voltage is reversed or either dot 
location is changed. 

Combining the voltage and current ratios, (27) and (28), 

V 2 I 2 = VA 

and we see that the primary and secondary complex volt-amperes are equal. 
The magnitude of this product is usually specified as a maximum allow- 

458 Two-port Networks 

able value on power transformers. If the load has a phase angle 6, 

Zi = \Z L \ll 

then V 2 leads I 2 by an angle 0. Moreover, the input impedance at the 
terminals of L x is Z t /a 2 , and thus Vj also leads l x by the same angle 0. 
If we let the voltage and current represent rms values, then we see that 
|V 2 ||I 2 | cos must equal IVjHI-J cos 0, and all the power delivered to the 
primary terminals reaches the load; none is absorbed by or delivered to 
the ideal transformer. 

The characteristics of the ideal transformer which we have obtained 
have all been determined by frequency-domain analysis. They are certainly 
true in the sinusoidal steady state, but we have no reason to believe that 
they are correct for the complete response. Actually, they are applicable 
in general, and the demonstration that this statement is true is much simpler 
than the frequency-domain analysis we have just completed. Our analysis, 
however, has served to point out the exact nature of approximations which 
must be made on a more exact model of an actual transformer in order 
to obtain an ideal transformer. For example, we have seen that the re- 
actance of the secondary winding must be much greater in magnitude than 
the impedance of any load which is connected to the secondary. Some 
feeling for those operating conditions under which a transformer ceases 
to behave as an ideal transformer is thus achieved. 

Returning to the circuit shown in Fig. 15-12 and the two equations, 
(18) and (19), describing it, we may solve the second equation for di 2 /dt 
and substitute into the first equation, 

di 1 M M 2 dij 

dt _ 

However, for unity coupling, M 2 = L X L 2 , and thus 

M [L~. 1 

C l = T v 2 = Vr "2 = — c 2 

2 2 

The relationship between primary and secondary voltage is thus found to 
apply to the complete time-domain response. 

An expression relating primary and secondary current is most quickly 
obtained by dividing (18) throughout by L v 

Dj di x M di 2 di 1 di 2 
L t dt h x dt dt dt 

and then invoking one of the hypotheses underlying the ideal transformer: 
L x must be infinite. If we assume that v t is not infinite, then 

459 Magnetically Coupled Circuits 

di x 

di 2 




= —at, + A 

where A is a constant of integration which does not vary with time. Thus, 
if we neglect any direct currents in the two windings and fix our attention 
only on the time-varying portion of the response, 

The minus sign arises, of course, from the placement of the dots and 
selection of the current directions in Fig. 15-12. 

The same current and voltage relationships are obtained in the time 
domain as were obtained previously in the frequency domain, provided 
that dc components are ignored. The time-domain results are more general, 
but they have been obtained by a less informative process. 

The characteristics of the ideal transformer which we have established 
may be utilized to simplify circuits in which ideal transformers appear. 
Let us assume, for purposes of illustration, that everything to the left of 
the primary terminals has been replaced by its Thevenin equivalent, as 
has the network to the right of the secondary terminals. We thus consider 
the circuit shown in Fig. 15-17. Excitation at any complex frequency s 
is assumed. 

Th6venin's or Norton's theorems may now be used to achieve an 
equivalent circuit which does not contain a transformer. For example, let 
us determine the Thevenin equivalent of the network to the left of the 
secondary terminals. Open-circuiting the secondary, I 2 = and therefore 
Ij = (remember L x is infinite). No voltage appears across Z gl , and thus 
Vj = V sl and V 2oc = a\ sl . The Thevenin impedance is obtained by killing 
V sl and utilizing the square of the turns ratio, being careful to use the 
reciprocal turns ratio since we are looking in at the secondary terminals. 
Thus, X th2 = Z gl a 2 . As a check on our equivalent, let us also determine 
the short-circuit secondary current l 2sc . With the secondary short-circuited, 

Fig. 15-17 The networks connected to the primary and secondary terminals 
of an ideal transformer are represented by their Thevenin equivalents. 

V ..(D 

t- % i 


k = 1 


Fig. 15-18 The Thevenin equivalent of the network to the left of the 
secondary terminals in Fig. 15-17 is used to simplify that circuit. 

the primary generator faces an impedance of Z 9l and, therefore, \ = 
Vjj/Zpj. Thus, I 2sc = — V sl /aZ 9l . The ratio of the open-circuit voltage 
to the short-circuit current is — a 2 Z ffl , as it should be. The Thevenin 
equivalent of the transformer and the primary circuit is shown in the circuit 
of Fig. 15-18. 

Each primary voltage may therefore be multiplied by the turns ratio, 
each primary current divided by the turns ratio, and each primary im- 
pedance multiplied by the square of the turns ratio, these modified voltages, 
currents, and impedances replacing the given voltages, currents, and 
impedances plus the transformer. If either dot is interchanged, the equiva- 
lent may be obtained by using the negative of the turns ratio. 

A similar analysis of the transformer and the secondary network shows 
that everything to the right of the primary terminals may be replaced by 
an identical network without the transformer, each voltage being divided 
by a, each current being multiplied by a, and each impedance being divided 
by a 2 . A reversal of either winding corresponds to the use of a turns ratio 
of —a. 

As a simple example of this application of equivalent circuits, consider 
the circuit given in Fig. 15-19. Let a — 10. The input impedance is 
10,000/100, or 100 fi. Thus Ij = 0.25 A, V x = 25 V, and the source 
delivers 12.5 W, of which 6.25 W is dissipated in the internal resistance 
of the source and 6.25 W is delivered to the load. This is the condition 
for maximum power transfer to the load. If the secondary circuit and the 
ideal transformer are removed by the use of the Thevenin equivalent, the 
simplified circuit of Fig. 15-20a is obtained. The primary current and 
voltage are now immediately evident. If, instead, the network to the left 

Fig. 1 5-19 A simple circuit in which a resistive load is matched to the source 
impedance by means of an ideal transformer. 

io kn 


toe n 

10 kn 

Fig. 15-20 The circuit of Fig. 15-19 is simplified by replacing (a) the trans- 
former and secondary circuit by its Thevenin equivalent and [b] the transformer 
and primary circuit by its Thevenin equivalent. 

of the secondary terminals is replaced by its Thevenin equivalent, the 
simpler circuit of Fig. 15-20& is obtained. The presence of the minus sign 
on the equivalent source should be verified. The corresponding Norton 
equivalents may also be obtained easily. 

Drill Problems 

15-10 The primary voltage of an ideal power distribution transformer is 4600 V 
rms, the turns ratio is 0.05, and parallel loads are connected to the secondary, 
one drawing 11.5 kW at unity PF and the other 9.2 kW at 0.6 PF lagging. Find 
the rms current amplitude in: (a) the lagging load; (b) the unity PF load; (c) the 

Am. 5.23; 50; 66.7 A 

15-11 Find the turns ratio a for the transformer in the circuit of Fig. 15-21 
so that: (a) the power delivered to the 10-S2 resistor is 25 per cent of that delivered 
to the 2-fl resistor for any independent sinusoidal source connected to x-y; (b) 
^2 = % when an independent source V, is connected to x-y; (c) the input resist- 
ance at x-y is 8 U. 

Ans. 1.38 or 3.62; 4.47; 24.0 

Fig. 15-21 See Drill Prob. 75-1!. 


462 Two-poit Networks 

15-12 A Thevenin source, 40/0° V rms in series with 50 fi, is connected to the 
primary of an ideal transformer, turns ratio of 1 : 2. The primary of a second ideal 
transformer, turns ratio 1 : 5, is connected to the secondary of the first transformer. 
The load at the output is 3000 &. Find the load power if: (a) the circuit is as 
described; (b) a 100-fi resistor is inserted in series with the primary of the second 
transformer; (c) a 100-fi resistor is connected across the primary of the second 

tranSformer - Ans. 2.45; 4.35; 7.50 W 


□ 1 The physical construction of three pairs of coupled coils is shown in Fig. 15-22. 
Show two different possible locations for the two dots in each pair of coils. 

Fig. 1 5-22 See Prob. 1 . 

□ 2 Find v 2 (t) in the circuit shown in Fig. 15-23 and sketch it as a function of 

Fig. 15-23 See Probs. 2 and 12. 

463 Magnetically Coupled Circuits 

□ 3 In the circuit shown in Fig. 15-24, find: (a) v ac (t); (b) «„,,(*); (c) ^(t). 


6H b 
-vJUULr o 



Rg. 15-24 See Prob. 3. 

□ 4 Find i x , t 2 , and v in the circuit shown in Fig. 15-25. Assume that the average 
value of iy(t) is zero. 

2 cos 100( 

Fig. 15-25 See Prob. 4. 

□ 5 It is possible to arrange three coils physically in such a way that there is mutual 
coupling between coils A and B and between B and C, but not between A and 
C. Such an arrangement is illustrated in Fig. 15-26. Find v a (t) if x-y is: (a) left 
open-circuited; (b) short-circuited. 

Fig. 15-26 See Prob. 5. 

□ 6 Determine values for C and M in the circuit shown in Fig. 15-27 so that the 
input impedance Z o6 has a pole at <o = 1 rad/s and a zero at <o = 2 rad/s. 

Fig. 1 5-27 See Prob. 6. 

464 Two-poit Network* 

□ 7 In the circuit shown in Fig. 15-3a, L, = 2H, L, = 5H, M = 3H, and 
v 1 — u 2 = 15 sin 6f V. Find i t (t) and « 2 (t). 

D 8 For the circuit shown in Fig. 15-28, determine I 2 (s) and sketch: (a) jl 2 (er)| versus 

a; (b) |I 2 (/w)| versus w. 

M = !H 

ioa!°(A) i.5 n< ih 



Fig. 1 5-28 See Probs. 8 and 1 7. 

D 9 Find V (s) for the circuit shown in Fig. 15-29. Identify all critical frequencies 
on the jai axis. 

M - 2 H 

Fig. 15-29 See Prob. 9. 

D 10 If i x and i 2 both enter dot-marked terminals of a pair of coupled coils for 
which L t = 20 mH, L 2 = 60 mH, and M = 30 mH, find the maximum instan- 
taneous energy storage if: (a) i x — i 2 = 0.6 cos ut A; (b) i x — —i 2 = 0.6 cos ait A; 
(c) ij = 2t 2 = cos oit A; (d) i t = cos ait, i 2 = 0.5 sin ait A. 

□ 1 1 The only energy stored in the circuit of Fig. 15-30 at t = is 5 mj in the 
capacitor. At what time is the energy stored in the magnetic fields of the coils 
a maximum, and what is its magnitude? 

Fig. 1 5-30 See Prob. 1 1 . 
1 H 



465 Magnetically Coupled Circuits 

□ 12 The source shown in Fig. 15-23 is replaced with a current source, i t = 
4 cos 10 4 t A. (a) Find v 2 (t). (b) How much energy is dissipated in any one 

□ 13 Two coupled coils are inside a sealed box with the ends brought out to 
terminals A, B, C, and D. Assume the coils are lossless. A voltage source, 
v„ = 10 cos 400f V, is applied as v AS and the resultant current is (y 240 ) sin 400f A, 
while v CD = 20 cos 400t V. If C and D are then short-circuited, the short-circuit 
current into D is (%„) sin 400t A. Find: (a) L AB ; (b) M, including identification 
of the dot-marked terminals; (c) L CD . 

□ 14 With reference to the circuit illustrated in Fig. 15-10, find i t (t) if the mutual 
inductance is: (a) 0; (b) 0.8 H; (c) 2 H, but with the dot located at the lower end 
of the 4-H coil. 

□ 1 5 The value of i at t = in the circuit illustrated in Fig. 15-31 is 50 mA. 
Find i(t) for t > 0. 

30 n 


20 mH" 

• r 


ao n 

Fig. 15-31 See Prob. 15. 

□ 1 6 A sinusoidal source, 10/0° V rms at o> = 1 krad/s, is connected to the 
primary of a linear transformer and a 3-fi resistor is across the secondary. Let 
Li = 1 mH, L 2 = 4 mH, and the coefficient of coupling be k. Plot a graph of 
the average power delivered to the 3-fl resistor as a function of k. 

□ 1 7 Refer to the circuit shown in Fig. 15-28 and determine the Thevenin equiva- 
lent of the network to the left of the 3.5-S2 resistor at a complex frequency s. 
Use the equivalent circuit to find I 2 (/2). 

□ 1 8 In the circuit shown in Fig. 15-32, the switch closes at t = 0. Find v 2 (t) 
for * > 0. 

15-32 See Prob. 18 

466 Two-perl Network* 

D 19 Let C x = C 2 = 0.1 y.F,L l =L 2 = l mH, and R x = R 2 = 2 Q, in the trans- 
former shown in Fig. 15-33. Determine |I | at w = 10 5 rad/s as a function 
of k, find the value of k that leads to maximum current amplitude, and sketch |I | 
versus k. 

Fig. 15-33 See Prob. 19. 

□ 20 Show how two transformers may be used to match a generator having a 
Thevenin equivalent impedance of 2800 + p Q to a load consisting of three 8-S2 
speakers, two of which must be supplied with equal power while the third receives 
50 per cent more than either of the other two alone. Draw a suitable circuit 
and specify the required turns ratios. 

D 21 Find the average power dissipated in each of the three resistors in the circuit 
of Fig. 15-34. 

Fig. 15-34 See Prob. 21. 
□ 22 The circuit shown in Fig. 15-35 contains two ideal transformers. Find l r 
Fig. 15-35 See Prob. 22. 

200 za°v( ~ 

467 Magnetically Coupled Circuits 

□ 23 A transformer having primary and secondary inductances Lj and 1^ and a 
coefficient of coupling k has a 1-juF capacitor as load. Assume that there are no 
resistances associated with any element. To show the effect of noninfinite L x and 
L 2 and nonunity k on the ideal transformer approximations, find the equivalent 
input capacitance at w = 10 4 rad/s for the following cases: (d)L x ~ oo, L 2 = oo, 
k = l.-ZVATj = 2;(fe)L 1 = 0.1 H,L 2 = 0.4 H,k = 1;^)^ = 0.1 H,L 2 = 0.4 H, 
k = 0.99. 

□ 24 A transformer whose nameplate data is 2300/230 V, 25 kVA, operates with 
primary and secondary voltages of 2300 V and 230 V rms, respectively, and can 
supply 25 kVA from its secondary winding. If this transformer is supplied with 
2300 V rms and is connected to secondary loads requiring 5 kW at 0.9 PF lagging 
and 12 kW at 0.8 PF lagging: (a) How many kilowatts of lighting load can it 
still supply? (b) What is the primary current? 

^f^QBWl;Beh¥«Fk lfiwiia»-.lwo pairs erf tetp^^pmpx&gfyi jfe&M *e . j 
l^jb^ieHriaafc" (t^pbdH "out^^iEMSiik" ft'awsy injpartant- ■ 

-tio^l jssteHtf, ttaniaxfcfrHi and dtetjribatkw sygHJflBB, or <jtjb^ $jesj?S& in 
.'.^^^^^fectrfcal st^wl or electrical i^hecg^t^i^ts *ke i^itteiiniha}s,N; 
^tt,i^i^%«»'|iy-^Jpietw(wfe, and kaves vi»'A»4>titpat teeaaiaak The 
'o&tpWttoniinal pair s^ very wen com^ert ^SiA 1^ i^wt terminal pair 

(a) (6) 

Fig. 16-1 (a) A one-port network, (b) A two-port network. 

of another network. A pair of terminals at which a signal may enter or 
leave a network is called a port, and a network having only one such pair 
of terminals is called a one-port network, or simply a one port. When more 
than one pair of terminals is present, the network is known as a multipart 
network. A one-port network is shown in Fig. 16-la, and the two-port 
network to which this chapter is principally devoted is shown in Fig. 16-lfo. 
We shall assume that sources and loads are connected directly across the 
two terminals of a port; for example, we should not expect any device to 
be connected between terminals a and c of the two-port network in Fig. 
16-lfo. If such a circuit must be analyzed, general loop or nodal equations 
should usually be written. 

The special methods of analysis which are developed for two-port net- 
works, or simply two ports, emphasize the current and voltage relation- 
ships at the terminals of the networks and suppress the specific nature of the 
currents and voltages within the networks. Our introductory study should 
serve to acquaint us with a number of important parameters and their use 
in simplifying and systematizing linear two-port network analysis. 


Some of the introductory study of one- and two-port networks is accom- 
plished best by using a generalized network notation and the abbreviated 
nomenclature for determinants introduced in Appendix 1. Thus, if we write 
a set of loop equations, 

Znli + Z 12 I 2 + Z13I3 + • • • + Zi^I* = Vj 

^11*1 "I" ^12*2 t" ^13*3 -»■■••+ ^ufljf = Vj 

Z 2 lll + Z^Ij + Z 23 I 3 + • • ■ + Zjjyljy = Vj 

^lll + Z 32 I 2 + Zggig + • • • + Zjyly = Vj 


ZjVlIl + Z OT I 2 + Zy 3 I 3 + • ■ • -(- 'Z, Iif/ I N — Vy 

then the coefficient of each current will be an impedance Z y (s), and the 
circuit determinant, or determinant of the coefficients, is 


470 Two-port Networks 

A, = 


Z 12 

Z 13 

Z 1JV 

Z 2i 

Z 22 

Z 23 

■ ■ Z 2tf 

Z 31 

Z 32 

Z 33 

' Z 3W 

Z W3 

Z iWV 


where 2V loops have been assumed, the currents appear in subscript order 
in each equation, and the order of the equations is the same as that of 
the currents. We also assume that Kirchhoff's voltage law is applied so 
that the sign of each Z ti term (Z u , Z 22 , . . . , Z m ) is positive; the sign of 
any Z v (i jt j) or mutual term may be either positive or negative, depending 
on the reference directions assigned to I 4 and L,. 

The use of minor notation (Appendix 1) enables the input or driving- 
point impedance at the terminals of a one-port network to be expressed 
very concisely. The result is also applicable to a two-port network if one 
of the two ports is terminated in a passive impedance. 

Let us suppose that the one-port network shown in Fig. 16-2a is 
composed entirely of passive elements and dependent sources; linearity is 
also assumed. An ideal voltage source V x is connected to the port, and 
the source current is identified as the current in loop 1. By the familiar 
procedure, then, 

Ii = 


Z 12 

Z 13 

Z l» 

Z 22 

Z 23 

' ^2N 

Z 32 

Z 33 

• Z 3tf 

Z AT2 

Z W3 ' 

• Z iW 

Z u 

Z 12 

Z 13 

■ ' Z 1AT 

z 2i 

Z 22 

Z 23 

Z 2W 

Z 31 

Z 32 

Z 33 

• Z 3W 

Z M 

Z W2 

Z W3 

' • Z AW 

or, more concisely, 

T - VA 


Z -^ 


Fig. 16-2 (a) An ideal voltage source V 1 is connected to the single port of a 
linear one-port network containing no independent sources; Z in = A z /A n . 
\b) A resistive one port used as an example, (c) A one port containing a 
dependent source used as an example. 



For the one-port resistive network shown in Fig. 16-2fo, 



-3 -1 


\i = 


= 34 


Z in = ^ = 3.21 Q 



Upon changing the circuit by including a dependent source, Fig. 16-2e, 
the three mesh equations are written, 



-21, + 7I 2 - I 3 = 

-31, - I 2 + 4I 3 = -2I„ = -2(1, 

6 -2 -3 

A z = -2 7 -1 =93 

-1 -3 4 


472 Two-port Networks 


7 -1 
-3 4 

= 25 

Z* = 9 %5 = 3-72 Q 

Drill Problems 

16-1 Connect an ideal source V,, with its positive reference at the upper 
terminal, to the circuit shown in Fig. 16-2fe, and show that: (a) A 12 = — 13; 

(b) I 2 = -V S A 12 /A z; (c) I 3 = VA 3 /A Z . 

Ans. Proof 

16-2 Find the input impedance presented to an ideal source by the network 
of Fig. 16-3 if the source is inserted in series with the: (a) 1-0 resistor; (b) 3-J2 
resistor; (c) 4-fi resistor. 

Ans. 3.80; 5.00; 6.70 fi 







Fig. 16-3 See Drill Prob. 16-2. 

1 6-3 Using the reference node and node-to-reference voltages indicated in Fig. 
16-4, write the three necessary systematic equations and find the input admittance 
presented to an ideal source connected between node 1 and the reference by: 
(a) evaluating A Y /A 11(Y ); (b) determining the reciprocal of Z jn = A Z /A 11(Z) ; 
(c) combining elements. 

Ans. 15/46; 15/46; 15/46 m® 

Fig. 16-4 Element values are given in mO; see Drill Prob. 16-3. 
V, ... V, ... V. 



0.4 4 


473 Two-port N«twofk» 


Let us now turn our attention to two-port networks. We shall assume in 
all that follows that the network is composed of linear elements and contains 
no independent sources; dependent sources are permissible. Further con- 
ditions will also be placed on the network in some special cases. 

We shall consider the two port as it is shown in Fig. 16-5; the voltage 
and current at the input terminals are V x and I v and V 2 and I 2 are specified 
at the output port. The directions of Ij and I 2 are both customarily selected 
as into the network at the upper conductors (and out at the lower conduc- 
tors). Since the network is linear and contains no independent sources 
within it, I t may be considered to be the superposition of two components, 
one caused by V x and the other by V 2 . When the same argument is applied 
to I 2 , we may begin with the set of equations 

ii = yu^ + y 12 v 2 (4) 

h = y 2 i v i + y 22 v 2 (5) 

where the y's are no more than proportionality constants, or unknown 
coefficients, for the present. They are called the y parameters and they 
are defined by (4) and (5). 

The most useful and informative way to attach a physical meaning to 
the y parameters is through a direct inspection of (4) and (5). Consider 
(4), for example; if we let V 2 be zero, then we see that y n must be given 
by the ratio of Ij to V r We therefore describe y n as the admittance 
measured at the input terminals with the output terminals short-circuited 
(V 2 = 0). Since there can be no question as to which terminals are short- 
circuited, y u is best described as the short-circuit input admittance. Alter- 
natively, we might describe y u as the reciprocal of the input impedance 
measured with the output terminals short-circuited, but a description as 
an admittance is obviously more direct. It is not the name of the parameter 
that is important; rather it is the conditions which must be applied to (4) 
or (5), and hence to the network, that are most meaningful; when the 
conditions are determined, the parameter can be found directly from an 
analysis of the circuit (or by experiment on the physical circuit). Each of 

Fig. 16-5 A general two port with terminal voltages and currents specified. 
The two port is composed of linear elements, including dependent sources, 
but not containing any independent sources. 


4 l 2 






v 2 

474 Two-port Networks 

the y parameters may be described as a current-voltage ratio with either 
Vj = (the input terminals short-circuited) or V 2 = (the output terminals 
short-circuited) : 





Because each parameter is an admittance which is obtained by short- 
circuiting either the output or input port, the y parameters are known as 
the short-circuit admittance parameters. The specific name of y u is the 
short-circuit input admittance, y 22 is the short-circuit output admittance, 
and y 12 and y 21 are the short-circuit transfer admittances. 

Consider the resistive two port shown in Fig. 16-6a. The values of the 
parameters may be easily established by applying (6) to (9), which we 
obtained directly from die defining equations (4) and (5). To determine 
y n , we short-circuit the output and find the ratio of I x to V 1 . This may 
be done by letting \ 1 = 1 V, for then y n = I 1 . By inspection of Fig. 16-6a, 
it is apparent that 1 V applied at the input with the output short-circuited 
will cause an input current of (% + y i0 ), or 0.3 A. Hence, 





v 2 

' Vi 


y 2i 

I 2 

'v 2 


y 22 

I 2 

1 V, 

= n 


= 0.3 n 

In order to find y 12 , we short-circuit the input terminals and apply 1 V 
at the output terminals. The input current flows through the short circuit 
and is — y i0 A. Thus 

y 12 = -o.i o 

By similar methods, 

y 21 = -0.1 y 22 = 0.15 15 

The describing equations for this two port in terms of the admittance 
parameters are, therefore, 

I, = 0.3V, - 0.1V 2 (10) 

I 2 = -0.1V, -)- 0.15V 2 (11) 

Fig. 16-6 (a) A resistive two port, (b) The resistive two port is terminated 
with specific one ports. 

In order to see what use might be made of such a system of equations, 
let us now terminate each port with some specific network. As a simple 
example, shown in Fig. 16-6fo, let us connect a general current source to 
the input port and a resistive load to the output port. A relationship must 
now exist between V x and I x at the input port because a specific network 
is present. This relationship may be determined solely from this external 
circuit. If we apply KirchhofF's current law (or write a single nodal 
equation) at the input, 

I x = 15 - 0.1 Vj 
For the output, Ohm's law yields 


Substituting these expressions for Ij and I 2 into (10) and (11), we have 

15 = 0.4V! - 0.1V 2 
= -O.lVj + 0.4V 2 

from which are obtained 


476 IWe-pert Networks 

The input and output currents are also easily found, 

Ij = 11 A I 2 = -2.5 A 

and the complete terminal characteristics of this resistive two port are then 

The advantages of two-port analysis do not show up very strongly for 
such a simple example, but it should be apparent that once the y param- 
eters are determined for a more complicated two port the performance 
of the two port for different terminal conditions is easily determined; it 
is only necessary to relate V 1 to I t at the input and V 2 to I 2 at the output. 

In the example just concluded, y 12 and y 21 were both found to be 
—0.1 0. It is not difficult to show that this equality is also obtained if 
three general impedances Z A , Z B , and Z c are contained in this it network. 
It is somewhat more difficult to determine the specific conditions which 
are necessary in order that y 12 = y 21 , but the use of determinant notation 
is of some help. Let us see if the relationships (6) to (9) can be expressed 
in terms of the impedance determinant and its minors. 

Since our concern is with the two port and not with the specific 
networks with which it is terminated, we shall let \ 1 and V 2 be represented 
by two ideal voltage sources. Equation (6) is applied by letting V 2 = 
(thus short-circuiting the output) and finding the input admittance. The 
network now, however, is simply a one port, and the input impedance of 
a one port was found in the previous section. We select mesh 1 to include 
the input terminals and let I t be that mesh current; we identify ( — L>) as 
the mesh current in mesh 2 and assign the remaining loop or mesh currents 
in any convenient manner. Thus, 

Z I - A * 

z, inlV 2 =0 — T — 

and, therefore, 


y 22 = ¥- ( 13 ) 


In order to find y 12 , we let V x = 0, and find Ij as a function of V 2 . We 
find that I t is given by the ratio 

477 Two-port Network! 


z 12 

Z 1JV 

-v 2 





^iV2 ' 


(-V 2 )A 2 





In a similar manner, we may show that 

_ A 1; 

y 2 i - A 


The equality of y 12 and y 21 is thus contingent on the equality of the two 
minors of A z , A. 12 and A 21 . These two minors are 

Z 21 


Z 24 




A 12 = 







Their equality is shown by first interchanging the rows and columns of one 
minor, say A 21 , an operation which any college algebra book proves is valid, 
and then letting every mutual impedance Zy be replaced by Z ;J . Thus, 
we set 

Mj-t •> — **9 


This equality of Zy and 2.^ is certainly obvious for the three passive 
elements, the resistor, capacitor, and inductor, and it is also true for mutual 

4Z8 Two_ P ort Network* 

inductance, as we proved in the preceding chapter. However, it is not 
true for every type of device which we may wish to include inside a 
two-port network. Specifically, it is not true in general for a dependent 
source, and it is not true for a device which is found in some microwave 
circuits, the gyrator. This device, over a narrow range of radian fre- 
quencies, provides an additional phase shift of 180° for a signal passing from 
the output to the input over that for a signal in the forward direction, 
and thus y 12 = — y 21 . 

Any device for which Z^ = Z ;i is called a bilateral element, and a circuit 
which contains only bilateral elements is called a bilateral circuit. We have 
therefore shown that an important property of a bilateral two port is 

yi2 = y 2 i 

and this property is glorified by stating it as the reciprocity theorem: 

In any passive linear bilateral network, if the single voltage source V, in branch 
* produces the current response I y in branch y, then the removal of the voltage 
source from branch x and its insertion in branch y will produce the current 
response I y in branch x. 

A simple way of stating the theorem is to say that the interchange of 
an ideal voltage source and an ideal ammeter in any passive linear bilateral 
circuit will not change the ammeter reading. 

If we had been working with the admittance determinant of the circuit 
and had proved that the minors A 21 and A 12 of the admittance determinant 
A Y were equal, then we should have obtained the reciprocity theorem in 
its dual form: 

In any passive linear bilateral network, if the single current source I x between 
nodes * and x' produces the voltage response V y between nodes y and y', 
then the removal of the current source from nodes x and x' and its insertion 
between nodes y and y' will produce the voltage response \ y between nodes 
x and x'. 

In other words, the interchange of an ideal current source and an ideal 
voltmeter in any passive linear bilateral circuit will not change the volt- 
meter reading. 

Two ports containing dependent sources receive emphasis in the follow- 
ing section. 

479 Two-port Networks 

Drill Problems 

16-4 By applying the appropriate 1-V sources and short circuits to the resistive 
two port of Fig. 16-7, determine; (a) y lt ; ib) y 12 ; (c) y 22 . 

An*. -% 4 ; % 4 ; % 4 

412 2(2 

o W\. — t VW 

+ I + 

•in v 2 


Fig. 1 6-7 See Drill Prob. 1 6-4. 

1 6-5 With reference to the ir network of Fig. 16-8, determine Z. A , Z B , and Z c 
so that y n = 100 /iU, y 22 = 500 /tf5, and y 12 = y 21 = — 200 /i®. 

Ans. -10; 3.33; 5 ktt 

o • */^V — i o 

Fig. 16-8 See Drill Prob. 16-5. 

1 6-6 Find y n , y 12 , and y 21 for the network of Fig. 16-9. 

Ans. -%; -y i2 ; %, 

h^ 2a 4Q *}} Ji 

o VVA — ? — W\ <C3^ — ° 

Fig. 16-9 See Drill Prob. 16-6. 


The two basic equations which determine the short-circuit admittance 

ii = yuVx + y 12 v 2 (16) 

i 2 = ygiVi + y 22 v 2 (17) 

480 Two-port Networks 

have the form of a pair of nodal equations written for a circuit containing 
two nonreference nodes. The determination of an equivalent circuit that 
leads to (16) and (17) is made more difficult by the inequality, in general, 
of y 12 and y 21 ; it helps to resort to a little trickery in order to obtain a 
pair of equations which will possess equal mutual coefficients. Let us add 
and subtract y 12 Vj (the term we would like to see present in the second 
equation above) on the right side of (17), 

! 2 = yi2 v i + y 2 2 v 2 + (y 2 i - y i2 ) v i 


(y 2 i - yi 2 ) v i = yi 2 v i + y 22 v 2 


The right sides of (16) and (19) now show the proper symmetry for a 
bilateral circuit; the left side of (19) may be interpreted as the algebraic 
sum of two current sources, one an independent source I 2 entering node 
2, and the other a dependent source (y 21 — y^)^ leaving node 2. 

Let us now "read" the equivalent network from (16) and (19). We first 
establish the reference node, and then a node labeled V t and one labeled 
V 2 . From (16), we establish the current I x flowing into node 1, we supply 
a mutual admittance (— y 12 ) between nodes 1 and 2, and we supply an 

Fig. 16-10 (a) and [b) Two ports which are equivalent to any general linear 
two port. The dependent source in (a) depends on Vj, and that in [b] depends 
on V 2 . (c) An equivalent for a bilateral network. 





(y 21 - 



>U + 12 

y 22 + y i2 







X 2 


+ [ 

/Spll - >i> ,V 3 

V l (■I) 

y il + >21 

y 22 + y 21 

V 2 





— — — 



— *■ 






^11 + 5-12 

y 22 + y 12 

V 2 


— ____ 





— WAr- 

l5oo a U,) iokn< 

0.0395 V,\ 

Fig. 16-11 The linear equivalent circuit of a transistor in common-emitter 
configuration with resistive feedback between collector and base. It is used 
as a two-port example. 

admittance between node 1 and the reference node of (y u + y 12 ). With 
V 2 = 0, the ratio of Ij to V t is then y n , as it should be. Now consider (19); 
we cause the current I 2 to flow into the second node, we cause the current 
(y 21 — Yi2l^i *° l eave the node, we note that the proper admittance ( — y 12 ) 
exists between the nodes, and we complete the circuit by installing the 
admittance (y 22 + y 12 ) from node 2 to the reference node. The completed 
circuit is shown in Fig. 16.10a. 

Another form of equivalent network is obtained by subtracting and 
adding y 2 iV 2 in (16); this equivalent circuit is shown in Fig. 16-10fo. 

If the two port is bilateral, then y 12 = y 21 , and either of the equivalents 
reduces to a simple -n network. The dependent source disappears. This 
equivalent of the bilateral two port is shown in Fig. 16- 10c. 

There are several uses to which these equivalent circuits may be put. 
In the first place, we have succeeded in showing that an equivalent of any 
complicated linear two port exists. It does not matter how many nodes 
or loops are contained within the network; the equivalent is no more 
complex than the circuits of Fig. 16-10. One of these may be much 
simpler to use than the given circuit if we are interested only in the terminal 
characteristics of the given network. We should also realize that linear 
transistor and vacuum-tube amplifiers must possess equivalent circuits in 
the form of Fig. 16-10a and b. 

As an example of the use of an equivalent circuit with a dependent 
generator, let us consider the two port shown in Fig. 16-11. This circuit 
may be considered as an approximate linear equivalent of a transistor circuit 
in which the emitter terminal is the bottom node, the base terminal is the 
upper input node, and the collector terminal is the upper output node; 
a 2000-fi resistor is connected between collector and base for some special 
application and makes the analysis of the circuit more difficult. 

There are two ways we might think about this circuit. If we recognize 
it as being in the form of the equivalent circuit shown in Fig. 16- 10a, then 
we may immediately determine the values of the y parameters. If recogni- 
tion is not immediate, then the y parameters may be determined for the 
two port by applying the relationships (6) to (9). We also might avoid any 
use of two-port analysis methods and write equations directly for the circuit 


482 Tw °-P ort Networks 

as it stands. Let us compare the network with the equivalent circuit. Thus, 
we first obtain 

and hence, 

y 12 = - Vzooo = -°- 5 m " 

yii = 1 / 5 oo-(- 1 /2ooo) = 2.5 mB 

and y 21 = 0.0395 + (-y 2000 ) = 39 mU 

The following equations must then apply: 

Ij = 2.5VJ - 0.5V 2 mA (20) 

I 2 = 39Vj + 0.6V 2 mA (21) 

where we are now using units of mA, m?5 , kS2, and V. We make use of 
these two equations by analyzing the performance of this two port when 
a current source of 1 /0° mA is provided at the input and a 0.5-kfi (2-mO ) 
load is connected to the output. The terminating networks thus give us 
the following specific information relating I x .to V 1 and I 2 to V 2 : 

I 2 = 1 I 2 = -2V 2 

Substituting into (20) and (21), we may obtain two equations relating Vj 
1 = 2.5VJ - 0.5V 2 = 39V! + 2.6V 2 

and V 2 : 


V t = 0.1 V V 2 = -1.5 V 
Ij = 1 mA I 2 = 3 mA 

From these data, it is easy to calculate the voltage gain 

G y = ^=-15 

the current gain 

483 Two-port Networks 

and, if sinusoidal excitation is assumed, the power gain 

f-, _ 'out _ ~ 12*2*2 _ AK 

p ~ T~ ~ vvi* ~ 

r in 12 "1*1 

The device might be termed either a voltage, a current, or a power 
amplifier, since all the gains are greater than unity. If the 2-M2 resistor 
were removed, the power gain would rise to 354. 

The input and output impedances of the amplifier are often desired 
in order that maximum power transfer may be achieved to or from an 
adjacent two port. The input impedance is the ratio of input voltage to 

Z jn =3 = 0.1 kil 

This is the impedance offered to the current source when the 500-S2 load 
is connected to the output. (With the output short-circuited, the input 
impedance is necessarily l/y u , or 400 Q.) It should be noted that the input 
impedance cannot be determined by replacing every source by its internal 
impedance and then combining resistances or conductances. In the circuit 
given, this procedure would yield a value of 416 fi. The error, of course, 
comes from treating the dependent source as an independent source. If 
we think of the input impedance as being numerically equal to the input 
voltage produced by an input current of 1 A, the application of the 1-A 
source produces some input voltage V ls and the strength of the dependent 
source (0.0395VJ) cannot be zero. We should recall that, when we obtain 
the Thevenin equivalent impedance of a circuit containing a dependent 
source along with one or more independent sources, we must replace the 
independent sources by short circuits or open circuits, but a dependent 
source must not be killed. Of course, if the voltage or current on which 
the dependent source depends is zero, the dependent source will itself be 
inactive; occasionally a circuit may be simplified by recognizing such an 

The output impedance is just another term for the Thevenin impedance 
appearing in the Thevenin equivalent circuit of that portion of the network 
faced by the load. In our circuit, which we have assumed driven by a 
1/OJl-mA current source, we therefore replace this source by an open 
circuit, leave the dependent source alone, and seek the input impedance 
seen looking to the left from the output terminals. This impedance may 
be found by several methods (none of which consists of combining all the 
elements in series or in parallel); let us apply 1/01 mA at the output 
terminals and determine V 2 . We place these requirements on (20) and (21), 
and obtain 

1 = 39Vj + 0.6V 2 

484 Two-port Networks 

and thus 

An alternative procedure might be to find the open-circuit output 
voltage and the short-circuit output current; the ratio is the Thevenin 
impedance or Z out . With an input current I x = 1 mA and with the load 
short-circuited (V 2 = 0), we find that 

Ij = 1 = 2.5V! - I 2 = 39Vi -(- 
and thus 

Again, with Ij = 1 mA and with the output open-circuited (I 2 = 0), we 

1 = 2.5V t - 0.5V 2 = 39V t + 0.6V 2 
and V 2oc = -1.857 V 

The assumed directions of V 2 and I 2 therefore result in a Thevenin or output 

as before. 

We now have enough information to enable us to draw the Thevenin 
or Norton equivalent of the two port of Fig. 16-11 (driven by a l /0° -mA 
current source and terminated in a 500-fl load, although this termination 
is of no consequence in the output equivalent circuits) as offered to the 
500-fi load. The Thevenin and Norton equivalents offered to the current 

Fig. 16-12 (a) The Norton equivalent of the network (Fig. 16-11) to the 
left of the output terminals, with Ii = 1 /Q° mA. [b) The Thevenin equivalent of 
that portion of the network to the right of the input terminals, if I2 = — 2V 2 mA. 

+ + 

15.6 mA (&) 119 £2? V 2 V, > 100 tl 


485 Two-port Network* 

source are also readily drawn. Thus, the Norton equivalent presented to 
the load must contain a current source equal to the short-circuit current 
I 2sc in parallel with the output impedance; this equivalent is shown in Fig. 
16- 12a. The Thevenin equivalent offered to the 1 /0° -mA input source must 
consist solely of the input impedance, as drawn in Fig. 16-12&. 

Drill Problems 

16-7 H the 2000-fl resistor is removed from the circuit of Fig. 16-11, if I t = 
1 /0° mA, and if a 500-fl resistor is installed at the output, find: (a) G r ; (b) G,; 
(c) G P . 

Ans. -18.8; 18.8; 354 

16-8 A two port is described by the following parameters: y u = 5 C, y 12 = 
-1!5, y 21 = 30 «, and y 22 = 1.5 «. Find the power gain G P = (- 1 / 2 V 2 I 2)/ 
(/W*) if: (°) r i = i/P-l A, and an output load, R L = % Q, is used; (b) Ij = 
1 /0° A and I 2 = 0.5 /0° A; (c) a source 0.2/QZ V in series with a 0.1-fi resistor is 
connected to the input and R L = 0.5 fl. 

Ans. 6.88; 10.0; 10.8 

16-9 For the circuit shown in Fig. 16-13, find: (a) y 12 ; (b) Y jB if V 2 = -4^; 

( C )Y ou( ifV 1 = 0. 

Ans. -%,• %; "/ 130 

Fig. 16-13 See Drill Probs. 16-9, 16-10, and 16-16. 


The concept of two-port parameters has been introduced in terms of the 
short-circuit admittance parameters. There are other sets of parameters, 
however, and each set is associated with a particular class of networks for 
which its use provides the simplest analysis. We shall consider only two 
other types of parameters, the open-circuit impedance parameters which 
are the subject of this section and the hybrid parameters which are discussed 
in the following section. 

486 Two-port Networks 

We begin again with the general linear two port which does not contain 
any independent sources; the currents and voltages are assigned as before 
(Fig. 16-5). Now let us consider the voltage V x as the response produced 
by two current sources Ij and I 2 . We thus write for V x 

and for V 2 

V x = «iA + Z12I2 (22) 

V 2 = z^ + z 22 I 2 (23) 

Of course, in using this pair of equations it is not necessary that I x and 
I 2 be current sources; nor is it necessary that V x and V 2 be voltage sources. 
In general, we may have any networks terminating the two port at either 
end. As the equations are written, we probably think of V x and V 2 as given 
quantities, or independent variables, and Ij and I 2 as unknowns, or de- 
pendent variables. The various ways in which two equations may be written 
to relate these four quantities define the different systems of parameters. 
The most informative description of the z parameters, defined in (22) 
and (23), is obtained by setting each of the currents equal to zero. Thus 


Since zero current results from an open-circuit termination, the z param- 
eters are known as the open-circuit impedance parameters. They are easily 
related to the short-circuit admittance parameters by solving (22) and (23) 
for Ij and I 2 : 

Ix = 

or I, = ( 5« W + ( -^ ) V 2 

\ Z U X 22 Z 12 Z 21' ^ X 11 I 22 ~ *12h\' 

Using determinant notation, and being careful that the subscript is a 
lowercase z, we assume that \ ^ and obtain 

211 = 17 

li 2 =o 

z -^ 

''12 — T 

l 2 


V 2 

Z 21 — T 

li 2 =o 

V 2 

222 — T 
l 2 


| V i 

Z 12 

lv 2 


l z ii 

Z 12 1 


I 22< 



487 Two ~P arl Networks 

A 1t A. 

yu = -^ yiz 


and from solving for I 2 , 

y 2i - - -^- y22 - ^ 

In a similar manner, the z parameters may be expressed in terms of the 
admittance parameters. Transformations of this nature are possible between 
any of the various parameter systems, and quite a collection of occasionally 
useful formulas may be obtained. We shall not specifically consider any 
other transformations. 1 

If the two port is a bilateral network, reciprocity is present; it is easy 
to show that this results in the equality of z 12 and z 21 . 

Equivalent circuits may again be obtained from an inspection of (22) 
and (23); their construction is facilitated by adding and subtracting either 
z 12 I 1 to (23) or ZjjjL, to (22). Each of these equivalent circuits contains 
a dependent voltage source. 

Let us leave the derivation of such an equivalent to Prob. 15 and con- 
sider next an example of a rather general nature. Can we construct a 
general Thevenin equivalent of the two port, as viewed from the output 
terminals? It is necessary first to assume a specific input circuit configura- 
tion, and we shall select an independent voltage source V s in series with 
a generator impedance Z g . Thus 

v s = v x + ia 

Combining this result with (22) and (23), we may eliminate V x and I ls and 

V ^1 y i (, "12^1 )i 

z,, + Z„ \ z n + A,/ 

The Thevenin equivalent circuit may be drawn directly from this equation; 
it is shown in Fig. 16-14. The output impedance, expressed in terms of 
the z parameters, is 

7 — , _ Z 12 z 21 

z ll + Z J 
"Except in the problems. 

Fig. 16-14 The Thevenin equivalent of a general two port, as viewed from 
the output terminals, expressed in terms of the open-circuit impedance 

If the generator impedance is zero, the simpler expression 

■7 _ Z 11 Z 22 ~ Z 12 Z 21 _ ^z _ * /"7 _ n^ 

""- ^ -^-^ (z '- } 

is obtained. For this special case, the output admittance is identical to 
y 22 , as indicated by the basic relationship of (9). 

As a numerical example, let us use a set of impedance parameters 
representative of a transistor operating in the grounded-emitter configura- 

z u = io 3 a z 12 = 10 q 

Zjj = - 10 6 a z 22 = 10 4 8 

and we shall consider the two port as driven by an ideal sinusoidal voltage 
source V, in series with a 500-fi resistor and terminated in a 10-kii load 
resistor. The two describing equations are 

\ = 10% + 10I 2 (28) 

V 2 = -10% + 10% (29) 

and the characterizing equations of the input and output networks are 

V 8 = 500^ + V, (30) 

V 2 =-10% (31) 

From these last four equations, we may easily obtain expressions for V 1? 
I 1 , V 2> and I 2 in terms of V s , 

V 1 = 0.75V S I 1= V - 



Iz _ '40 


489 T we-perl N«twerk> 

From this information, it is simple to determine the voltage gain, 

the current gain, 

the power gain, 

G v = IJ = -333 

G, = ^ = 50 

— V V I* 

G - = -4ir = 16 ' 700 

and the input impedance, 

^ = 1500 a 

The output impedance may be obtained by referring to Fig. 16-14, 

z ll + *■» 

Drill Problems 

16-10 For the circuit shown in Fig. 16-13, find: (a) z 12 ; (b) z^; (c) z^. 

Am. 4,- i0; 13 Q 

16-1 1 The admittance parameters of a bilateral two port are: y u = 0.25 Z5, 
y = -0.05 IS, y 22 = 0.1 V. Find: (a) z u ; (&) z 21 ; (c) z^. 

Aw. »%;«%,■"% 

16-12 The T-equivalent circuit of a transistor in the common-base arrangement 
is shown in Fig. 16-15. Find: (a) z u ; (fo) z 12 ; (c) z^. 

Ans. r b ; r„ + r^ r b + ar c 

Fig. 16-15 See Drill Probs. 16-12, 16-13, and 16-15. 


o VA- 


-VA — A- 

490 Two-porf Network! 

16-13 For the transistor considered in Drill Prob. 16-12 and Fig. 16-15, let r e = 
20 fi, r h = 800 0, r c = 500 M2, and a = 0.98. A current source, I x = 2 mA, is 
applied at the input and a load, R L = 10 kfi, is connected to the output. Find: 
(a) G, = I 2 /I i; (b) G v = V 2 /V i; (c) G P = -G ; G r . 

Ans. -0.96; 180; 187 


The use of the hybrid parameters is well suited to transistor circuits because 
these parameters are among the most convenient to measure experimentally 
for a transistor. The difficulty in measuring, say, the open-circuit impedance 
parameters arises when a parameter such as z 21 must be measured. A known 
sinusoidal current is easily supplied at the input terminals, but because of 
the exceedingly high output impedance of the transistor circuit, it is difficult 
to open-circuit the output terminals and yet supply the necessary dc biasing 
voltages and measure the sinusoidal output voltage. A short-circuit current 
measurement at the output terminals is much simpler to instrument. 

The hybrid parameters are defined by writing the pair of equations 
relating \ v I v V 2 , and I 2 as if \ 1 and I 2 were the independent variables: 

V x = h,A + hi 2 V 2 (32) 

I 2 = h,^ + h 22 V 2 (33) 

The nature of the parameters is made clear by first setting V 2 = 0, 

V I 

h u = -j-M = short-circuit input impedance 


v 2 =o 

and h 21 = -2- = short-circuit current gain 

l i lv 2 =o 

and then letting I x = 0, 

V I 
h 12 = — U = open-circuit reverse voltage gain 

V 2 I li=0 

and h 22 = ^-\ = open-circuit output admittance 

V 2 'li=0 

Since the parameters represent an impedance, an admittance, a voltage 
gain, and a current gain, it is understandable that they are called the 
"hybrid" parameters. 

In order to illustrate the ease with which these parameters may be 
evaluated, consider the bilateral resistive circuit drawn in Fig. 16-16. With 





6 a 


Fig. 16-16 A bilateral network for which the h parameters are found; 

h 12 = -^l' 

the output short-circuited (V 2 = 0), the application of a 1-A source at the 
input (I x = 1 A) produces an input voltage of 3.4 V (V 1 = 3.4 V); hence, 
h n = 3.4 ft. Under these same conditions, the output current is easily 
obtained by current division, I 2 = —0.4 A; thus, h 21 = —0.4. The re- 
maining two parameters are obtained with the input open-circuited 
(I x = 0). Let us apply a voltage of 1 V at the output terminals (V 2 — 1 V). 
The response at the input terminals is 0.4 V (Vj = 0.4 V), and thus 
h 12 = 0.4. The current delivered by this source at the output terminals 
is 0.1 A (I 2 - 0.1 A), and therefore h^ =0.10. It is a consequence of 
the reciprocity theorem that h 12 = — h^ for a bilateral network. 

The circuit shown in Fig. 16-17 is a direct translation of the two defining 
equations (32) and (33). The first represents Kirchhoff's voltage law about 
the input loop, while the second is obtained from Kirchhoff's current law 
at the upper output node. This circuit is also a popular transistor equivalent 
circuit. Let us assume some reasonable values for the common-emitter 
configuration: h n = 1200 0, h 12 = 2 X 10" 4 , \ x = 50, \ 2 = 50 X 10" 6 
?5 , an input voltage source of 1/QZ. mV in series with 800 £2, and a 5-k£2 
load. For the input, 

10" 3 = (1200 + 800)l! + 2 x 10- 4 V 2 

and at the output, 

I 2 = -2 x 10" 4 V 2 = 50l! + 50 X 10" 6 V 2 

Fig. 16-17 The four h parameters are referred to a two port. The pertinent 
equations are: Vj = h 11 I 1 + b 12 V 2 , Ig = h 21 I 1 + h 2 2 V 2- 



492 Two-port Network! 


Ii = 0.510 juA 
I 2 = 20.4 M A 

V 1 = 0.592 mV 
V 2 = - 102 mV 

Through the transistor we have a current gain of 40, a voltage gain of 
— 172, and a power gain of 6880. The input impedance to the transistor 
is 1160 0, and a few more calculations show that the output impedance 
is 22.2 k£2. 

Drill Problems 

16-14 For a bilateral two port, y n = 0.5 V, y 12 = -0.4 y, and y 22 = 0.6!!. 
Find: (a) h n ; (b) h 21 ; (c) h 22 . 

Ans. -0.8; 0.28 IS; 2 a 

16-15 For the transistor T-equivalent circuit of Fig. 16-15, let r e = 20 a, 
r b = 800 Q, r c = 500 ka, and a = 0.98. Find: (a) h 12 ; (b) h 21 ; (c) h 22 . 

Arts. -0.98; 2 X 10~ 6 !i; 1.6 X 10~ 3 

16-16 For the circuit shown in Fig. 16-13, find: (a) h n ; (b) h 12 ; (c) h 21 . 

Ans. -y 13 ; %,- «% 3 a 

16-17 For the two port terminated as shown in Fig. 16-18, find the average 
power: (a) supplied by the 1-V sinusoidal source; (b) delivered to the 10-a load 
resistor; (c) lost in the 5-a internal resistance of the source. 

Ans. 4; 20; 200 mW 

hn=40tl h.,= 0.4 

h 21 =10 h,,= 0.1B 

Fig. 16-18 See Drill Prob. 16-17. 

"10 n 


□ 1 The three rows of a determinant are in order: 9, —2, —3; —2, 6, —1; and 
— 3, —1, 4. (a) Find the input impedance offered to a source appearing in only 
the first mesh, assuming that the determinant is A z (values in ohms), (b) Suppose 

493 ^ wo "P°'t Networks 

that the reference direction for I 2 had been selected in the opposite direction 
so that the three rows of the determinant A z were 9, 2, —3; 2, 6, 1; —3, 1, 4; 
repeat part (a), (c) Find the input impedance offered to a source connected 
between the first node and the reference node, assuming that the original deter- 
minant is A y (values in mhos). 

□ 2 (a) Find the input impedance of the one port illustrated in Fig. 16-19. (b) 
If a 10- V dc source is connected to the input terminals, find the power absorbed 
by each element. 


Fig. 16-19 See Prob. 2. 

□ 3 The admittance determinant of a circuit is given by 

4 -;2 -1 + /2 

-/2 1 + ;3 ,1 

-1 + /2 ft 2 

Find the average power supplied by a source, 2 /0° A, connected between node 
1 and the reference node. 

□ 4 The reciprocity theorem also holds for the complete response, forced plus 
natural, if there is no initial-energy storage This restriction is necessary because 
the network must be passive, except for the single source specified. Demonstrate 
the truth of this extension of the reciprocity theorem by: (a) finding v c in the 
circuit shown in Fig. 16-20 for t < and t > 0; (b) interchanging the step-current 
source and the (instantaneous) voltmeter and finding the voltmeter response for 
t < and t> 0. 

Fig. 16-20 See Prob. 4. 

494 Two-port Networks 

□ 5 Measurements made on a two-port network yield the following data: for 
Vj = -5 V and V 2 = -8V,I,= -9 A and I 2 = - 17 A; and for V 1 = -8 V 
and V 2 = —5 V, I x = — 30 A and I 2 = 4 A. (a) Find the four short-circuit 
admittance parameters, (b) Find I 1; I 2 , and V 2 if V 1 = 10 V and a 2-S2 resistor 
is connected to the output port. 

□ 6 Find the four short-circuit admittance parameters for the circuit shown in 
Fig. 16-21. 

Fig. 16-21 See Probs. 6 and 21. 

D 7 Two two ports, identified by a and b subscripts, have y parameters y 11(J> y 116 , 
y 12o> etc. Find the y parameters for the overall network if the output of net- 
work a is connected directly to the input of network b. 

□ 8 Find the y parameters for the: (a) w network shown in Fig. 16-22o; (b) T 
network shown in Fig. 16-22b. (c) Show that the corresponding y parameters for 
the two networks are equal if: 

rr Z a Z 6 z _ Z 1 Z 2 + Z 2 Z 3 + Z 3 Z 1 

z» = 

Z a 

+ Z*+Zc 



+ Z 6 + Z c 

z,z a 

z 3 - Zo + z» + z c z < - 

z 2 

ZjZ 2 


Z 2 Z 3 

+ Z 3 Z 1 

Z 3 

ZjZ 2 


Z 2 Z 3 

+ Z 3 Z 1 

Z ! 


z 2 

— wv ° 

V, 2„ 

Fig. 16-22 See Prob. 8. 

□ 9 Given the equivalence between ir and T networks expressed by the rela- 
tionships in part (c) of Prob. 8, transform: (a) the ir network of Fig. 16-23a to 

495 Two-port Networks 

a T network; (b) the T network of Fig. 16-236 to a it network; (c) the one ports 
of Fig. 16-23c and d to single resistor equivalents. 


v, 20 n ; 





f— W T VNA — , 
I in I in I 

<in <m <ic 

— VW- 1 — WV— ' 

id I in 

— VW— — WV— ' 

I in I in I 
£in ?in ?iq 

1 — VW-1 — VA— 1-^ 

in in 


Fig. 16-23 See Prob. 9. 

D 10 Figure 16-24o shows the equivalent circuit of a vacuum-tube circuit called 
a cathode follower, famous for its relatively low output impedance. Determine 
the output impedance for this cathode follower and compare it to that for a typical 
vacuum-tube amplifier, as illustrated by the equivalent circuit of Fig. 16-246. 
Let g„, = 2 mtS, r„ = 10 kft. 




«-. v l 

Fig. 16-24 See Prob. 10. 

D11 Determine the short-circuit admittance parameters for the circuit of: (a) Fig. 
16-25o; (6) Fig. 16-256. 



(a) (b) 

Fig. 16-25 See Probs. 11, 16, and 22. 

□ 12 Measurements on a linear two-port network show that y u = 2y 22 = 0.1 U, 
and y 21 = — 10y 12 = 0.4 V . How do these values change if a 10-fi resistor is 
installed: (a) across the input terminals? (b) across the output terminals? (c) in 
series with the input? (d) in series with the output? 

□ 13 A linear two port for which y n = 2 a, y 12 = -0.5 S, y 21 = 20 V, and 
y 22 = 0.4 ^ is terminated in R L . A 5-V sinusoidal source in series with 1 Si is 
connected to the input. For each part below, determine the value of R L required 
to maximize the magnitude of the specified quantity, and give the maximum value 
of that quantity: (a) V 2 ; (b) I 2 ; (c) P 2av ; (d) V r 

□ 14 Obtain expressions giving the open-circuit impedance parameters in terms 
of the short-circuit admittance parameters. 

□ 1 5 Determine values for the elements shown in Fig. 16-26 if the circuit is to 
be equivalent to any circuit described by: \ = z n Ij + z 12 I 2 > V 2 = z 2i J i + z 22*2- 

( )I 2 


-W\ o 

( ) L. ( ) 
:< ) 

Fig. 1 6-26 See Prob. 1 5. 

□ 1 6 Determine the open-circuit impedance parameters for the circuit of: (a) Fig. 
16-25a; (b) Fig. 16-256. 

□ 17 A three-terminal network, with terminals labeled a, b, and c, is operated 
as a two-port network by connecting a to 1, b to V and 2', and c to 2, as shown 
in Fig. 16-27. For this arrangement z n = 10 U, z 12 = 2 SI, z 21 = -2 fi, and 
Z2 2 = 6 fi. Find the z parameters that result from connecting: (a) b to 1, c to 
1' and 2', and a to 2; (fe) c to 1, a to 1' and 2', and £> to 2. 

497 Two-port Networks 

□ 18 A two port is connected as shown in Fig. 16-28. Obtain an expression for: 
(a) the voltage gain, G v = V 2 /V i; (b) the current gain, G 7 = I 2 /I i; (c) the input 
impedance, Z jn = V^; (d) the power gain, G p = (% Re V 2 IJ)/(y 2 Re V^), for 
a pure-resistance network; (e) the output impedance Z th . 


Fig. 16-28 See Prob. 18. 

1 9 For the circuit shown in Fig. 16-29: (a) determine R G so that the generator 
is matched (R G = R in ) to the two port when R L = 4 U; (b) determine R L so that 
R L is matched (R L = R th ) to the two port when R G = 6 fi; (c) determine R t and 
fl G so that matched conditions are achieved simultaneously at the input and 
the output. 

Fig. 16-29 See Prob. 19. 

□ 20 The most convenient measurements on a certain two-port device are the 
following: the open-circuit forward- voltage gain is —20; the short-circuit for- 
ward-current gain is 1000; the open-circuit input impedance is 10 kfi; and the 
short-circuit input impedance is 8 kS2. Find the four z parameters. 

□ 21 

The ABCD parameters are denned by V 1 = AV 2 - BI 2 , I x = CV 2 - DI 2 . 

(a) Find the values of these parameters for the network shown in Fig. 16-21. 

(b) What condition is forced on these parameters when the network is reciprocal? 

□ 22 Determine the hybrid parameters for the circuit of: (a) Fig. 16-25a; (b) Fig. 

□ 23 Express each of the four hybrid parameters in terms of the admittance 

□ 24 Consider a transistor whose h parameters for common-base operation are 
h n = 50 G,h 12 = 3 X lO" 3 ,^! = -0.98, and \ 2 = 4 x 10~ 6 W. This transistor 
is to be used as a voltage amplifier between a 2-kQ load and a 10-mV source 
having an internal resistance of 100 Q. (a) Determine the load voltage, (b) The 
transistor is installed backwards; assuming that it does not burn out, find the load 

498 Tw °-P° rt Networks 

D 25 A simplified linear equivalent circuit for a good transistor used at audio 
frequencies in the common-emitter arrangement is shown in Fig. 16-30. Two 
identical two ports are used in cascade (output of first connected directly to input 
of second). If the combination is terminated in R L — 10 kti, and h u = 10 3 fl, 
h 21 = 102, „ 22 = io-5 0> find Vj /V x . 




: h 2 2(a> 

^21 *!. 


Fig. 16-30 See Prob. 25. 
□ 26 Find the four h parameters for the circuit shown in Fig. 16-31. 

? — O- 




Fig. 16-31 See Prob. 26. 

D 27 Find the h parameters for the parallel connection of two two ports, as 
illustrated in Fig. 16-32. 

o + 

Fig. 16-32 See Prob. 27. 

□ 28 Scraps from an old lab notebook of Ben Franklin's apparently describe 
a network for which: ". . . transistor . . . bias . . . i%i = — 160 . . . h 12 = 0.2 
. . , y 22 = y 200 . . . z 12 = 2. . . ." Determine the open-circuit forward-voltage 
gain and the short-circuit reverse-current gain for this device. 




M^* JsBSe5Kilw«:i- , 'j j 


ta this chapter we continue our introduction to circuit analysis by extending 
the froqiionc\ -domain concept to include forum; .mil i-i-sinmse?"' 
which are not in general. sinusoids, exponentials, or damped sinusoids. ()ur 
goa) is a generalization of the process of determining the lon-ed response. 
The complete response of a linear circuit to an arbitrary forcing function 
is composed of the sum of a forced response and a natural response. The 
natural response was initially considered in Chaps. 5 to 7 but, with few 
receptions, only simple series or parallel RL, RC, and RLC circuits were 
*xainined. However, *e complex-frequency concept in Chap. 13 provided 

504 Network Analysis 

us with a general method of obtaining the natural response; we discovered 
that we could write the form of the natural response after inspecting the 
pole-zero constellation of an appropriate immittance or transfer function 
of the network. Thus, a powerful general method for determining the 
natural response became available. 

Now let us consider our status with respect to the forced response. 
We are able to find the forced response in any purely resistive linear circuit, 
regardless of the nature of the forcing function, but this can hardly be 
classed as a scientific breakthrough. If the circuit includes energy-storage 
elements, then we can find the forced response only for those circuits and 
forcing functions to which we can apply the impedance concept; that is, 
the forcing function must be direct current, exponential, sinusoidal, or 
damped sinusoidal. This is the barrier which we seek to breech in this 

We shall begin by considering forcing functions which are periodic and 
have functional natures which satisfy certain mathematical restrictions that 
are characteristic of any function which we can generate in the laboratory. 
Any such function may be represented as the sum of an infinite number 
of sine and cosine functions which are harmonically related. Therefore, 
since the forced response to each sinusoidal component may be determined 
easily by sinusoidal steady-state analysis, the response of the linear network 
to the general periodic forcing function may be obtained by superposing 
the partial responses. 

Some feeling for the validity of representing a general periodic function 
by an infinite sum of sine and cosine functions may be gained by considering 
a simple example. Let us first assume a cosine function of radian frequency 

U 1 (f) =r 2 COS U t 


«o = 2,7 /o 

and the period T is 

T _ J_ _ 2ot 
/o "o 

The harmonics of this sinusoid have frequencies ruc , where w is the 
fundamental frequency and n = 1, 2, 3, . . . . The frequency of the first 
harmonic is the fundamental frequency. Next let us select a third harmonic 

v 3a(t) — cos 3^0* 

Fig. 17-1 Several of the infinite number of different waveforms which may 
be obtained by combining a fundamental and a third harmonic. The funda- 
mental is v 1 = 2 cos <*> * and the third harmonic is: [a) v^ = cos 3w f; [b] 
1334 = 1 .5 cos 3<o t; (c) Ugc = sin 3« £ 

The fundamental v^t), the third harmonic v^t), and the sum of these two 
waves are shown as functions of time in Fig. 17-la. It should be noted 
that the sum is periodic with period T = 2tt/« . 

The form of the resultant periodic function changes as the phase and 
amplitude of the third harmonic component change. Thus, Fig. 17-lfo shows 
the effect of combining v^t) and a third harmonic of slightly larger ampli- 

%,(f) = 1.5 cos 3u t 


506 "«lw»tk Analysis 

By shifting the phase of the third harmonic, 

the sum, shown in Fig. 17- lc, takes on a still different character. In all 
cases, the period of the resultant waveform is the same as the period of 
the fundamental waveform. The nature of the waveform depends on the 
amplitude and phase of every possible harmonic component, and we shall 
find it possible to generate waveforms which have an extremely nonsinus- 
oidal character by an appropriate combination of sinusoidal functions. 
After we have become familiar with the use of an infinite sum of sine 
and cosine functions to represent a periodic waveform, we shall consider 
the frequency-domain representation of a general nonperiodic waveform 
in the next chapter. 


We first consider a periodic function f(t) defined in Sec. 11-3 by the func- 
tional relationship 


where T is the period. We further assume that the function f(t) satisfies 
the following properties: 

1 f(t) is single-valued everywhere. 

2 The integral I \f(t)\ dt exists (i.e., is not infinite) for any 

choice of t . 

3 f(t) has a finite number of discontinuities in any one period. 

4 f(t) has a finite number of maxima and minima in any one period. 

We shall consider f(t) to represent a voltage or current waveform, and any 
voltage or current waveform which we can actually produce must satisfy 
these conditions. Certain mathematical functions which we might hy- 
pothesize may not satisfy these conditions, but we shall assume that the 
four conditions listed above are always satisfied. 

Given such a periodic function f(t), the Fourier theorem 1 states that 
f(t) may be represented by the infinite series 

x Jean-Baptiste Joseph Fourier published this theorem to 1822. Some rather unbelievable 
pronunciations of this French name come from American students; it should rhyme with 
"poor today." 

507 Fourier Analyst! 

f(t) = 00 + 0! cos u t + Oj cos 2u t + • • • + fcj sin co f + i> 2 sin 2w f + • ■ • 

= a + 2 ( a n cos «"o f + K sin "*><>') (1) 


where the fundamental frequency w is related to the period T by 


and where a and the a n and fe n are constants which depend upon n and 
f(t). Equation (1) is the trigonometric form of the Fourier series for f(t), 
and the process of determining the values of the constants a , a n , and b n 
is called Fourier analysis. Our object is not the proof of this theorem, but 
only a simple development of the procedures of Fourier analysis and a 
feeling that the theorem is plausible. 

Before we discuss the evaluation of the constants appearing in the 
Fourier series, let us collect a set of useful trigonometric integrals. We 
shall let both n and k represent any of the set of integers 1, 2, 3, ... . In 
the following integrals, we shall use and T as the integration limits, but 
it is understood that any interval of one period is equally correct. Since 
the average value of a sinusoid over one period is zero, 

f sin noi t dt = (2) 


r T 
and | cos noi t dt = (3) 

It is also a simple matter to show that the following three definite integrals 
are zero: 

j sin ku t cos rm t dt = (4) 


I sin ku t sin no> t dt = k / n (5) 


r T 

| cos ku t cos ruo f dt = k ^ n (6) 

Those cases which are excepted in (5) and (6) are also easily evaluated; 
we obtain 

X i 

sin 2 nu t dt = — (7) 

u <■ 

I cos 2 rm t dt = — (8) 

Jn 2 

508 N **w°rl< Analysis 

The evaluation of the unknown constants may now be accomplished 
readily. We first attack a . If we integrate each side of the Fourier series 
(1) over a full period, we obtain 

XT -T T « 

f(t) dt = J a dt + I ^ ( a n cos ""o* + ^n sin ""o') ^' 

,T ~T 

a dt + I 

"o J o „— 1 

But every term in the summation is of the form of (2) or (3), and thus 

f f(t) dt = a T 

l r T 
or a ° = JJ fV> dt ( 9 ) 

This constant a is simply the average value of f(t) over a period, and we 
therefore describe it as the dc component of f(t). 

To evaluate one of the cosine coefficients, say a k , the coefficient of 
cos kw t, we first multiply each side of (1) by cos ku t and then integrate 
both sides of the equation over a full period: 

I /(f) cos ko) t dt = I a cos ko) t dt + I "S] a n cos koi t cos nw t dt 
J o J o J o n=l 

T » 

+ | ^ fc n cos few f sin n4o f d( 

From (3), (4), and (6) we note that every term on the right side of the 
equation with one exception is zero. That term is evaluated by (8) and 
we obtain 

2 r T 
a k=YJ f(t) cos ku tdt (10) 

This result is twice the average value of the product f(t) cos ku t over a 

In a similar way, we obtain b k by multiplying by sin kus t, integrating' 
over a period, noting that all but one of the terms on the right side are 
zero, and performing that single integration by (7). The result is 

2 r T 
bk= TJ fW sinku o td t (11) 

which is twice the average value of f(t) sin ku t over a period. 

Equations (9) to (11) now enable us to determine values for a and all 
the a n and b n in the Fourier series (1). 

509 fouriw Analysis 

Let us consider a numerical example. The "half-sinusoidal" waveform 
shown in Fig. 17-2a represents the voltage response obtained at the output 
of a half- wave rectifier circuit, a nonlinear circuit whose function is to 
convert a sinusoidal input voltage to a (pulsating) dc output voltage. In 
order to represent this voltage as a Fourier series, we must first determine 
the period and then express the graphical voltage as an analytical function 
of time. From the graph, the period is seen to be 

and thus 

T = 0.4 s 

/„ = 2.5 Hz 
<o = 5w rad/s 

With these three quantities determined, we now seek an appropriate 
expression for f(t) or v(t) which is valid throughout the period. Obtaining 
this equation or set of equations proves to be the most difficult part of 
Fourier analysis for many students. The source of the difficulty is appar- 
ently either the inability to recognize the given curve, carelessness in 
determining multiplying constants within the functional expression, or 

Fig. 17-2 (fl| The output of a half-wave rectifier to which a sinusoidal input 
is applied, (fo) The discrete line spectrum of the waveform in (a). 





-=»« (s) 



0.5 V, 

0-4 V„ 
0.3 V m 

0.1 v m 




->/ (Hz) 

510 Network Analysis 

negligence in not writing the complete expression. In this example, the 
statement of the problem infers that the functional form is a sinusoid; the 
amplitude is V m , the radian frequency has already been determined as 5tt, 
and only the positive portion of the cosine wave is present. The functional 
expression for the period t — to t = 0.4 is therefore 


f V m cos 5wt < t < 0.1 

0.1 < t < 0.3 

V m cos 5vrt 0.3 < t < 0.4 

It is evident that -the choice of the period extending from t = —0.1 to 
t = 0.3 will result in fewer equations and, hence, fewer integrals: 

v(t) = f 

V„,cos5rt -0.1<t<0.1 

- - (12) 

.0 0.1 <t < 0.3 

This form is preferable, although either description will yield the correct 

The zero-frequency component is easily obtained: 

1 r - 3 
a »=0Al ^ dt 

1 r r 01 r - 3 1 

= 0A[L 1 v - cos5wtdt+ { 1 (0 H 

and 00 = -^ (13) 

Notice that the integral must be broken up into a number of integrals, 
each over a portion of the period, where each integral corresponds to one 
of die functional forms used to express v(t) over the complete period. 
The amplitude of a general cosine term is 

2 r 01 

VL cos Jwrt cos 5irkt dt 

The form of the function we obtain upon integrating is different when k 
is unity than it is for any other choice of k. If k = 1, we have 

«i = 5V m f ' cos 2 5vrf dt = ^1 (14) 

511 Fouriw Analysis 

whereas if k is not equal to unity, we find 

a k = 5V m I cos 5irt cos 5wkt dt 


= 5V m J y 2 [cos 5w(l + k)t + cos 5?r(l - k)t] dt 


57 1 — Ar 

Some of the details of the integration have been left out for those who 
prefer to work out the small tedious steps for themselves. It should be 
pointed out, incidentally, that the expression for a k when k ^ 1 will yield 
the correct result for k = 1 in the limit. 

A similar integration shows that all the b k are zero, and the Fourier 
series thus contains no sine terms. The Fourier series is therefore obtained 
from (13) to (15): 

V V 2V 2V 

Wt) = -=• + -H cos 5vt + — ^ cos 10« - — ^ cos 20wt 

+ -5^cos30n*- ■■■ (16) 

In Fig. 17-2a, t?(t)-is shown as a function of time; in (12), t>(t) is expressed 
as an analytical function of time. Either of these representations is a 
time-domain representation. Equation (16), the Fourier series repre- 
sentation of f(£), is also a time-domain expression, but it may be transformed 
easily into a frequency-domain representation. For example, we could 
locate the points in the s plane that represent the frequencies present in 
(16). The result would be a mark at the origin and symmetrical marks on 
the positive and negative /<o axis. A more customary method of presenting 
this information, and one which shows the amplitude of each frequency 
component, is by a line spectrum. A line spectrum for (16) is shown in 
Fig. 17-2£>; the amplitude of each frequency component is indicated by 
the length of the vertical line located at the corresponding frequency. We 
also speak of this spectrum as a discrete spectrum because any finite 
frequency interval contains only a finite number of frequency components. 

One note of caution must be injected. The example we have considered 
contains no sine terms, and the amplitude of the fcth harmonic is therefore 
\a k \. If b k is n ot zero, the n the amplitude of the component at a frequency 
kco must be ^/a k 2 + b k 2 . This is the general quantity which we must show 
in a line spectrum. When we discuss the complex form of the Fourier series, 
we shall see that this quantity is obtained more directly. 

512 Network Analysis 

The Fourier series obtained for this example includes no sine terms and 
no odd harmonics (except the fundamental) among the cosine terms. It 
is possible to anticipate the absence of certain terms in a Fourier series 
before any integrations are performed, by an inspection of the symmetry 
of the given time function. We shall investigate the use of symmetry in 
the following section. 

Drill Problems 

17-1 In the Fourier series for f(t), determine a 5 , b 5 , and Va^ 2 + b 2 if 
/(f) = : (a) 2, < f < 0.1; - 1, 0.1< f < 0.2; T = 0.2; (b) - 1, < f < 0.1; 
2, 0.1<f<0.2; T = 0.2; (c) 2, -0.05 < f < 0.05; - 1, 0.05 < t < 0.15; 
T = 0.2 

Ans. 0, -0.382, 0.382; 0, 0.382, 0.382; 0.382, 0, 0.382 

Fig. 17-3 See Drill Probs. 17-2 and 17-5. 





-> I (s) 

-> t («) 

> < (s) 

513 Fourier Analysis 

1 7-2 Write the Fourier series for the three voltage waveforms shown in 
Fig. 17-3. 

Ans. — (sin irt + — sin 3vt + — sin &nt + ■••)•' 
it 3 5 

4 11 

—(cos nt — - cos 3nt + — cos 5rrt — ■ ■ •); 
it 3 5 

O T 7 

— 5 (sin Tit — — sin 3irt + — — sin 5trt — ■ ■ ■ ) V 
it y 2io 


The two types of symmetry which are most readily recognized are even- 
function symmetry and odd-function symmetry, or simply even symmetry 
and odd symmetry. We say that f(t) possesses the property of even sym- 
metry if 



Such functions as t 2 , cos 3i, In (cos t), sin 2 It, and a constant C all possess 
even symmetry; the replacement of t by ( — t) does not change the value 
of any of these functions. This type of symmetry may also be recognized 
graphically, for if f(t) — f( — t) then mirror symmetry exists about the f(t) 
axis. The function shown in Fig. 17-4a possesses even symmetry; if the 
figure were to be folded along the f(t) axis, then the portions of the graph 

Fig. 1 7-4 (a) A waveform showing even symmetry, (b) A waveform showing 
odd symmetry. 










514 NMworic Analysis 

of the function for positive and negative time would fit exactly, one on 
top of the other. 

Now let us investigate the effects that even symmetry produces in a 
Fourier series. If we think of the expression which equates an even function 
f(t) and an infinite sum of sine and cosine functions, then it is apparent 
that the infinite sum must also be an even function. A sine wave, however, 
is an odd function, and no sum of sine waves can produce any even function 
other than zero (which is both even and odd). It is thus plausible that the 
Fourier series of any even function is composed of only a constant and 
cosine functions. Let us now show carefully that b k = 0. We have 

2 r T/2 

*>*=-/ f(t) sin ko> tdt 

2 T r° r T/2 1 

= t I /(') sia *"<>* dt + I /(*) sin *"o* dt 

Now let us replace the variable t in the first integral by — t, or r = —t, 
and make use of the fact that f(t) = f( — t) = /(t): 

2 r r° r T/2 1 

h=r -I /(-.T)sin(-fao T)dT+ / /(f)sinfao tdt 

l I •'t/2 J J 

2 r c Tn r T/2 1 

= — — I f[r) sin Kko t dr + J f(t) sin ku t dt 

But the symbol we use to identify the variable of integration cannot affect 
the value of the integral. Hence, 

b k =0 (18) 

Thus, no sine terms are present. A similar examination of the expression 
for a k leads to an integral over the half period extending from t = to 

t = %T: 

4 r T/2 
o» = 7 f(t) cos kUgtdt (19) 

The fact that a k may be obtained for an even function by taking "twice 
the integral over half the range" should seem logical. 

We define odd symmetry by stating that if odd symmetry is a property 
of f(t), then 

fit) = -f(-t) (20) 

515 Fouriar Analysis 

In other words, if t is replaced by (— t), then the negat ive of the given 
function is obtained; for example, t, sint, £cos70t, ty/1 + t 2 , and the 
function sketched in Fig. 17 -4b are all odd functions and possess odd 
symmetry. The graphical characteristics of odd symmetry are apparent 
if the portion of f(t) for t > is rotated about the positive t axis and the 
resultant figure is then rotated about the f(t) axis; the two curves will fit 
exactly, one on top of the other. That is, we now have symmetry about 
the origin, rather than about the f(t) axis as we did for even functions. 
A function having odd symmetry can contain no constant term or 
cosine terms in its Fourier expansion. Let us prove the second part of this 
statement. We have 

2 r T/2 
a k =—\ f(t) cos koi t dt 

1 •'-t/2 

2 T r° c Tn 1 
= — M f(t) cos ku t dt + I f(t) cos ku t dt 

1 L J -T/2 J J 

and we now let t — — t in the first integral, 

2 r r ° r T/2 1 

a k = t - I /(- T ) cos (-fcco T) dr + I /(*) cos ku tdt 

2 r r T 't ,- T/2 1 

= f\J /( - T ) cos ku T dr + J /(') cos fcw 0* dt \ 

But /( — t) = — /(t), and therefore 

a k = (21) 

A similar, but simpler, proof shows that 

Furthermore, the values for b k may again be obtained by integrating over 
half the range: 

K=^\ f(t)<dnh* tdt (22) 

1 J o 

Examples of even and odd symmetry are afforded by Drill Prob. 17-2, 
preceding this section. In both parts (a) and (b), a square wave of the same 
amplitude and period is the given function. The time origin, however, is 
selected to provide odd symmetry in (a) and even symmetry in (b), and 
the resultant series contain, respectively, only sine terms and cosine terms. 



» t 

n n 


> t 


Fig. 17-5 (a) A waveform somewhat similar to the one shown in Fig. 17-4a, 
but possessing half-wave symmetry, [b) A waveform somewhat similar to the 
one shown in Fig. W-Ab, but possessing half-wave symmetry. 

It is also worthwhile pointing out that the point at which t = could be 
selected to provide neither even nor odd symmetry; the determination of 
the coefficients of the terms in the Fourier series then takes twice as long. 
The Fourier series for either of these square waves also have one other 
interesting characteristic; neither contains any even harmonics. 2 That is, 
the only frequency components present in the series have frequencies which 
are odd multiples of the fundamental frequency; a h and b k are zero for 
k even. This result is caused by another type of symmetry, called half-wave 
symmetry. We shall say that f(t) possesses half-wave symmetry if 

f(t) = ~/(t - y 2 T) 

Except for a change of sign, each half cycle is like the adjacent half cycles. 
Half-wave symmetry, unlike even and odd symmetry, is not a function of 
the choice of the point t = 0. Thus, we can state that the square wave 
(Fig. 17-3a or b) shows half-wave symmetry. Neither waveform shown in 
Fig. 17-4 has half-wave symmetry, but the two somewhat similar functions 
plotted in Fig. 17-5 do possess half -wave symmetry. 

It may be shown that the Fourier series of any function which has 

2 Constant vigilance is required to avoid confusion between an even function and an even 
harmonic, or an odd function and an odd harmonic. For example, fe 10 is the coefficient of an 
even harmonic, and it is zero if f(t) is an even function. 


517 Fourier Analysis 

half-wave symmetry contains only odd harmonics. Let us consider the 
coefficients a k . We have again 

2 c Tn 
a k = ~ /(*) cos ku t dt 

1 J - T /2 

2 T r° r T/2 1 
= t\ /(*) cos ku »t dt + I f(t) cos *<o t dt 

I LJ-t/2 J J 

which we may represent as 

«* = f Ci + y 

Now we substitute the new variable t = « + %T into integral J^ 

'i = f /( T - % T ) cos fc<o (r - Y 2 T) dr 

C Tn ,, . / , k-> T ■ , ■ ko> o T \ J 

= I — /( T ) I cos ko> T cos — ^ 1- sin fao T sin I or 

But to T is 2t, and thus 

■ fcw o r • l n 

sin — £— = sin fcw = 


Ij = — cos few I /(t) cos ko> T dr 

After noting the form of J 2 , we therefore may write 

2 r Tn 

a k = — (1 — cos far) I /(f) cos ku tdt 

The factor (1 — cos tor) indicates that a k is zero if k is even. When k is 
odd, we have 

4 r r/2 
a * = t I /(*) cos ^V dt * odd ( 23 ) 

* "'o 

A similar investigation shows that b k is also zero for all even k, and when 
k is odd 

4 z- 772 
b k =- f(t) sin ku t dt k odd (24) 

518 Network Analysis 

It should be noted that half-wave symmetry may be present in a 
waveform which also shows odd symmetry or even symmetry. The wave- 
form sketched in Fig. 17-5a, for example, possesses both even symmetry 
and half-wave symmetry. Its Fourier series therefore contains only odd- 
harmonic cosine functions; the values oi'a k may be determined from (23) 
[once the functional form for f(t) is known]. It is always worthwhile 
spending a few moments investigating the symmetry of a function for which 
a Fourier series is to be determined. 

Drill Problems 

1 7-3 Sketch each of the functions described below and decide whether or not 
even symmetry, odd symmetry, and half-wave symmetry are present: (a) v = 10, 
0< t< l;t> = 20, 1 <t <2;v = -10,2 < t<3;v = -20,3 < t< 4; repeats; 
(b) v — 5t, -2 < t < 2; repeats; (c) v = 10 cos0.25flt, -2 < t < 2; repeats. 

Ans. Yes, no, no; no, yes, no; no, no, yes 

1 7-4 Determine the Fourier series for each of the functions described in Drill 
Prob. 3. 

2 4 » {-If nirt 20 .A 1 nirt 

Ans. > — = cos ——- ; > — cos nir sin — — ; 

t t £?, 4n 2 - 1 2 it „4l n 2 

y ( - I)<»+i"2 cos —— + sin 

^Vnir 2 nir 2 J 



Through the use of the Fourier series, we may now express an arbitrary 
periodic forcing function as an infinite sum of sinusoidal forcing functions; 
the forced response to each of these functions may be determined by 
conventional steady-state analysis; the form of the natural response may 
be determined from the pole-zero constellation of the appropriate network 
function; the initial conditions existing throughout the network, including 
the initial value of the forced response, enable the amplitude of the natural 
response to be selected; and, finally, the complete response is obtained as 
the sum of the forced and natural responses. Let us illustrate this general 
procedure by a specific example. 

We shall apply the square wave of Fig. 17-6a, which includes a dc 
component, to the series RL circuit, as shown in Fig. 17-6&. The forcing 
function is applied at t = 0, and the current is the desired response. Its 

-i 10 


X v t )r >r 
2 2 2 

-» * (s) 

Fig. 17-6 (a) A square-wave voltage forcing function, (b) The forcing 
function of (a) is applied to this series RL circuit at J = 0; the complete 
response i[t) is desired. 

initial value is zero. The forcing function has a fundamental frequency 
co = 2, and its Fourier series may be written down by comparison with 
the solution of Drill Prob. 17-2a: 

20 A sin2nt 

v(t) = 5 + — Y 

w »= ! " 

We shall find the forced response of the fcth harmonic by working in the 
frequency domain. Thus, 


V* = §(-/!) 

The impedance offered by the RL circuit at this frequency is 

Z k = 4 + j(2k)2 = 4 + j4k 
and thus the component of the forced response at this frequency is 

. V, _ -/5 

2* »*(1 + /*) 


520 N** w °H< Analysis 

Transforming to the time domain, we have 

h(t) = -, — h 1 ,- cos (2kt - 90° - tan" 1 k) 
irk yl 4- k 2 


ir(l + it 2 ) V k 

cos 2kt ) 

Since the response to the dc component is obviously 1.25 A, the forced 
response may be expressed as the summation 

-_ 5 ^, f sin2kt cos2fe] 

i f (t) = l.: 

The familiar natural response of this simple circuit is the single exponential 
term (characterizing the single zero of the input impedance) 

i„(t) = Ae-* 

The complete response is therefore the sum 

Ut) = i f (t) + i n (t) 

and, since t(0) = 0, it is necessary to select A so that 

A = -v(0) 

Letting t — 0, we find that i f (0) is given by 


Although we could express A in terms of this summation, it is more conve- 
nient to use the numerical value of the summation. The sum of the first 
5 terms of 21/(1 + k 2 ) is 0.671, the sum of the first 10 terms is 0.695, the 
sum of the first 20 terms is 0.708, and the exact sum 3 is 0.720 to three 
significant figures. Thus 

A = -1.25 + —0.720 = -0.104 

and i(t) = -0.104*-* + 1.25 + -f \ sin2kt - cos2kt ] 


3 The sum of this series is known in closed form: ^S 1 = — tanh — 

£i 1 + k 2 4 2 



» t (s) 

Fig. 1 7-7 The initial portion of the complete response of the circuit of 
Fig. 17-6fo to the forcing function of Fig. 17-6a. 

In obtaining this solution, we have had to use many of the most general 
concepts introduced in this and the preceding 16 chapters. Some we did 
not have to use because of the simple nature of this particular circuit, but 
their places in the general analysis were indicated above. In this sense, 
we may look upon the solution of this problem as a significant achievement 
in our introductory study of circuit analysis. In spite of this glorious feeling 
of accomplishment, however, it must be pointed out that the complete 
response, as obtained above in analytical form, is not of much value as 
it stands; it furnishes no clear picture of the nature of the response. What 
we really need is a sketch of i(t) as a function of time. This may be obtained 
by a laborious calculation at a sufficient number of instants of time; an 
available digital computer can be of great assistance here. It may be 
approximated by the graphical addition of the natural response, the dc term, 
and the first few harmonics; this is an unrewarding task. When all is said 
and done, the most informative solution of this problem is probably ob- 
tained by making a repeated transient analysis. That is, the form of the 
response can certainly be calculated in the interval from t = to t = 
w/2 s; it is an exponential rising toward 2.5 A. After determining the value 
at the end of this first interval, we have an initial condition for the next 
Y 2 it-s interval. The process is repeated until the response assumes a 
generally periodic nature. The method is eminendy suitable to this ex- 
ample, for there is negligible change in the current waveform in the 
successive periods it/2 < t < 3tt/2 and 3tt/2 < t < 5tt/2. The complete 
current response is sketched in Fig. 17-7. 


In obtaining a frequency spectrum, we have seen that the amplitude of 
each frequency component depends on both a k and b k ; that is, the sine 
term and the cosine term both contribute to the amplitude. The exact 


522 Network Anolysit 

expression for this amplitude is y/a k 2 + b k 2 . It is possible to obtain this 
amplitude directly by using a form of Fourier series in which each term 
is a cosine function with a phase angle; the amplitude and phase angle 
are functions of f(t) and k. An even more convenient and concise form 
of the Fourier series is obtained if the sines and cosines are expressed as 
exponential functions with complex multiplying constants. 

Let us first take the trigonometric form of the Fourier series: 

/(*) = °o + 2 ( a n cos nc V + K sin nu t) 


and then substitute the exponential forms for the sine and cosine. After 

2 +e 2 ) 

fit) = a a +±(e 

n=l v 

We now define a complex constant c n : 

c n = /iK - ;*„) (25) 

The values of a n , b n , and c n all depend on n and f(t). Suppose we now 
replace n by ( — n); how do the values of the constants change? The coeffi- 
cients a n and b n are defined by (10) and (11), and it is evident that 

°-n = a n 

but 6_ =~K 

From (25), then, 


c_ n = Y 2 (a„ + jb n ) (26) 

We may therefore express f(t) as 

»=1 n=l 

or /(() = ^ Cne in w t + 2 c_„ e -*"><>< 

n=0 n=l 

Finally, instead of summing the second series over the positive integers 
from 1 to oo, let us sum over the negative integers, from —1 to — oo: 

f(t) = 2 c n e>™°' + 2 c„e> n "°' 

n=0 n=-l 

or f(t) = 2 c„^'~»' (27) 

523 Fouriar Analysis 

Equation (27) is the complex form of the Fourier series for f(t); its concise- 
ness is one of the most important reasons for its use. In order to obtain 
the expression by which a particular complex coefficient c k may be evalu- 
ated, we substitute (10) and (11) into (25): 

I ~T/2 I ~T/2 

c * = ™ I /(*) cos ku t dt - \— I f(t) sin ku t dt 

I ■'_j. / 2 ' J -T/2 

use the exponential equivalents of the sine and cosine, and simplify: 

c k = ± C T/2 f(t)e-*»°' dt (28) 

1 J -T/2 

Thus, a single concise equation serves to replace the two equations required 
for the trigonometric form of the Fourier series. Instead of evaluating two 
integrals to find the Fourier coefficients, only one integration is required; 
moreover, it is almost always a simpler integration. It should be noted 
that the integral (28) contains the multiplying factor 1/T, whereas the 
integrals for a n and b n both contain the factor 2/T. 

Since the amplitude of the Fourier component at a frequency ko> is 
yja k 2 + b k 2 , the amplitude, expressed in terms of c k , must be 2|cJ. In 
other words, the magnitude of c k is equal to one-half the amplitude of the 
component of the frequency spectrum at the frequency ku . 

Let us consider a numerical example to illustrate the use of the complex 
form of the Fourier series. A train of rectangular pulses of amplitude V 
and duration r, recurring periodically every T s, is shown in Fig. 17-8a. 
The fundamental frequency is, therefore, 

fo = ~j 

In order to determine the line spectrum of v(t), we shall determine the 
c k first and then obtain the corresponding amplitudes of the frequency 
components by multiplying each |c k | by 2. The value of a general complex 
coefficient is first found from (28): 

1 r T/2 
1 *J~w/n 


to + T 

«-*"' dt 

V / c -fto)<i«o4-T) _ g-j*<oolo\ 

-iku T 

_f!0_ e -i*»„tt„+T/» sin (l/ 2 fao oT ) 

_ V t sin (y 2 ku T) ftMn( ,„ +r/2) 

t y 2 fao T 




.-. v„ 

o j r 


lc K l 

**— envelope 


/ = — 





Fig. 1 7-8 (a) A periodic sequence of rectangular pulses, (b) The correspond- 
ing discrete line spectrum. 

The magnitude of c k is therefore 

_ V I sin (y 2 fcu T) I 

r I y 2 fao T I 

and the angle of c k is 

angc t = — ku lt + -^-j (possibly plus 180°) 



The trigonometric factor in (29) occurs frequently in modern commu- 
nication theory, and it is called the sampling function. Thus, we define 

Sa(*) = S J>±* 

Because of the way in which it helps to determine the amplitude of the 
various frequency components in v(t), it is worthwhile discovering the 
important characteristics of this function. First, we note that Sa(x) is zero 
whenever x is an integral multiple of tt; that is, 

Sa(far) = k = 1, 2, 3, 


525 Feuriw Analyth 

When x is zero, the function is indeterminate, but it is easy to show that 
its value is unity: 

Sa(0) = 1 

The magnitude of Sa(x) therefore decreases from unity at x = to zero 
at x — tt. As x increases from tt to 2tt, |Sa(x)| increases from zero to a 
maximum less than unity, and then decreases to zero once again. As * 
continues to increase, the successive maxima continually become smaller 
because the numerator of Sa(x) cannot exceed unity and the denominator 
is continually increasing. 

Now let us return to the line spectrum of v(t). We may express (29) 
in terms of the fundamental cyclic frequency / : 

V | sin(far/ T) | 
1 fcl ~ T I hrf r I V ' 

The amplitude of any harmonic (at a frequency kf ) is obtained from (31) 
by using the known values t and T = l// and selecting the desired value 
of k. Instead of evaluating (31) at these discrete frequencies, let us sketch 
the envelope of \c k \ by considering the frequency kf to be a continuous 
variable. That is, /( = kf ) can actually take on only the discrete values 
of the harmonic frequencies / , 2/ , 3/ , and so forth, but we may think 
of k for the moment as a continuous variable. When / is zero, |c fc | is 
evidently V t/T, and when/has increased to 1/t, |c t | is zero. The resultant 
envelope is sketched as the broken line of Fig. 17-8b. The line spectrum 
is then obtained by simply erecting vertical lines at each harmonic fre- 
quency, as shown in the sketch. The amplitudes shown are those of the 
c k ; except for the dc component, the amplitudes of the corresponding 
sinusoids are twice as great. The particular case sketched applies to the 
case where t/T — l/(1.5v7) = 0.212. In this example, it happens that there 
is no harmonic exactly at that frequency at which the envelope amplitude 
is zero; another choice of t or T could produce such an occurrence, 

There are several observations and conclusions which we may make 
about the line spectrum of a periodic sequence of rectangular pulses. With 
respect to the envelope of the discrete spectrum, it is evident that the 
"width" of the envelope depends upon t, and not upon T. As a matter 
of fact, the shape of the envelope is not a function of T. It follows that 
the bandwidth of a filter which is designed to pass the periodic pulses is 
a function of the pulse width t, but not of the pulse period T; an inspection 
of Fig. 17-8b indicates that the required bandwidth is about 1/t Hz. If 
the pulse period T is increased (or the pulse repetition frequency / is 
decreased), the bandwidth 1/t does not change, but the number of spectral 

526 Network Analysis 

lines between zero frequency and 1/t Hz increases, albeit discontinuously; 
the amplitude of each line is inversely proportional to T. Finally, a 
shift in the time origin does not change the line spectrum; that is, |c t | 
is not a function of t . The relative phases of the frequency components 
do change with the choice of t . 

Drill Problem 

1 7-5 Determine the general coefficient c k in the complex Fourier series for each 
of the three waveforms shown in Fig. 17-3. 




co ^).- -i-j^2 HnJ f 


□ 1 A voltage waveform is defined by: v = 0, -T/2 < t < -d/2; v = 100, 
-d/2 < t < d/2; v = 0, d/2 < t < T/2. Express d in terms of T so that the 
amplitude of the kth harmonic component of the Fourier series is the maximum 
possible value. 

□ 2 The half-wave rectifier output shown in Fig. 17-2o is replaced by the full-wave 
rectifier output, such. that f(t + 0.2) = f(t). fcompare the discrete line spectrum 
with that shown in Fig. 17-26. 

D 3 (a) Show that the derivative of the triangular waveform of Fig. 17-3c is twice 
the value of the waveform of Fig. 17-36 for all t. (6) Show that the Fourier series 
for the two waveforms have a corresponding relationship. 

D 4 (a) Obtain the Fourier series for the waveform displayed in Fig. 17-9. (6) Find 
the sum of the first four terms of the series at t = 2. 

■> t 

Fig. 17-9 See Prob. 4. 

□ 5 The ideal voltage source v s (t), where v s (t) = — 5 + 10 cos (irt/S) for 
— 1 < t < 1 and zero elsewhere in the period interval — 2 < t < 2, is connected 

527 Fourier Analysis 

to the series combination of 100 Q, 40 juF, and 2.5 H. Find the ratio of the 
amplitude of the 64th harmonic to that of the fundamental for: (a) the source 
voltage; (b) the source current. 

□ 6 A rectangular current pulse of amplitude 20 mA, duration 5 ms, and period 
50 ms begins at t = 0. (a) Find the average power supplied to a 100-fl resistor 
by this current, (b) What fraction of the total power is represented by the dc 
component? (c) by the fundamental component? (d) by the fifth harmonic compo- 

□ 7 A square wave of voltage with a period of 4ot ms has an amplitude of ±4 V. 
Draw the discrete frequency spectrum of the current produced in a 50-mH 
inductor by this voltage. 

D 8 (a) Find the Fourier series for the current waveform of Fig. 17-10. (b) If this 
waveform is shifted 4 ms later (to the right) in time, determine the Fourier series. 


















t (ms) 

Fig. 17-10 See Prob. 8. 

□ 9 In the interval from t = to t = 3, f(t) is defined by the sketch of Fig. 17-11. 

(a) Define /(t) in the interval 3 < t < 6 so that/(t) is an odd function with T = 6. 

(b) Define /(t) in the interval 3 < t < 6 so that/(*) is an even function with T = 6. 

(c) Define f(t) in the interval — 9 < ( < so that f(t) is an odd function with 
half-wave symmetry with T = 12. Determine the Fourier series for the waveform 
of: (d) part (a); (e) part (b); (f) part (c). 



-> t 

Fig. 1 7-1 1 See Prob. 9. 

□ 10 Determine whether the given function is odd, even, or neither: (a) t/(t 2 + 1); 
(b) to" 2 '; (c) cos (sin 2f); (d) sin (cos 2*); (e) fsin|t|; (/) -0.5 + u(t); (g) /(«) + 
/(-') + 3. 

528 Network Analysis 

□ 1 1 Taking advantage of the symmetry present, determine the Fourier series for: 
(a) /(f) = sint,0<t< w/4; /(f) = cos t, ir/4<t< *r/2; T = w/2; (b) /(f) = 
for 2<f<6 and 10 < t < 14; /(f) = 100, -2<f<2; /(f) =-100, 
6 < t < 10; T = 16. 

D 12 Sketch an example of a waveform that has neither even, odd, nor half-wave 
symmetry, but whose Fourier series contains no cosine terms. 

□ 13 Determine the Fourier series for the waveforms shown in Fig. 17-12a and 
b, and sketch the line spectrum for each. 

Fig. 17-12 See Prob. 13. 

D M A Fourier series may be obtained for a waveform by numerical methods when 
an analytical expression for /(f) is not known or is unwieldy. The integral for 

2 r T 
a k=JJ f(t) cos ku t 


may be expressed as an approximate sum by subdividing the interval of integration 
into M equal parts: 

2 M T 2 ■ *■ ■ ■ 

% = f 2 f(tJ(cOS ko> t m ) -7T = TT 2 /(4) COS *<V™ 
mzzl m=rl 

The value of f(t m ) and cos ku> t m may be determined at the midpoint of each 
interval. A similar summation is used to evaluate b k . By dividing the period into 

529 Fouriar Analysis 

20 equal parts, find the approximate amplitude of the 1%-Hz component of the 
waveform described by: f(t) = 1/(1 - t), - 1 < t < 0, and f(t) = 1/(1 + *)>■ 
< t < 1, with T = 2. 

D 15 An ideal voltage source, an open switch, a 2-kfi resistor, and a 50-jiF capacitor 
are in series. The voltage waveform is a square wave similar to that shown in 
Fig. 17-3a, but with a peak-to-peak amplitude of 100 V and a period of 10 ms. 
The switch is closed at t = + and the resistor voltage is the desired response. 
(a) Work in the frequency domain of the feth harmonic to find the forced response 
to this component. Express the total forced response as a trigonometric Fourier 
series, (b) Specify the functional form of the natural response, (c) Determine the 
complete response. 

D 16 Find the complete response of the circuit described in Prob. 15 by considering 
the input as a sequence of suitable unit-step forcing functions. The response is 
to be determined and plotted over an interval which represents two periods of 
the forcing function. Can you show that the maximum and minimum values of 
the resistor voltage (forced response) are 51.25 and —51.25 V, respectively? 

D 17 A parallel RLC circuit is energized by a square-wave-current forcing function 
alternating between ±/ with a period of 0.5 ms. Specify the resonant frequency 
and Q of the RLC circuit if the current through the inductor is to be essentially 
a 150-kHz sinusoid. Assume that no other component of the inductor current 
may have an amplitude greater than 5 per cent of the desired component. 

□ 18 An AM (amplitude-modulated) broadcasting station operating at 920 kHz 
carries an exciting flute duet, with one flute playing A (440 Hz) and the other 
tootling C (512 Hz). For 40 per cent modulation by each signal, the voltage 
waveform applied to the antenna might be given by: v = 500(1 + 0.4 sin 880wf 

+ 0.4 sin 1024t7() cos 1.84 X lOSt V. Draw the discrete frequency spectrum for 
the voltage waveform and determine its rms value. 

□ 1 9 A pulsed communication signal consists of a burst of 250-kHz energy every 
1.25 ms that lasts 0.2 ms. Determine the frequency spectrum of this signal, noting 
the atmospheric pollution it produces. 

□ 20 Determine the complex Fourier series of the waveform illustrated in Fig. 

Fig. 17-13 See Prob. 20. 


-> t(s) 

530 Network Analysis 

□ 21 A periodic waveform is given by t(t) = Ae~ bt , < t < 1, with T = 1. By 
finding the complex Fourier series, show that the value of h that will maximize 
the amplitude of the 5-Hz component in the frequency spectrum is about 5.27. 

□ 22 A waveform having both odd and half-wave symmetry is specified by 
f(t) = It, — 1 < t < 1. Let T = 4; find the complex Fourier series and sketch 
the discrete frequency spectrum. 

Cliapi^ Eighteen 
Fourier ¥ransforms 


In this chapter we shall begin to consider the use of transform method 
in studying the behavior of linear circuits through a discussion of the Fourier 
transform. The Laplace transform is die subject of the next chapter. Before 
beginning a formal discussion, however, let us look back to Chap. 9. 

At that rime we recalled the facilitation of certain arithmetic operations 
(multiplication, division, extraction of roots, and raising numbers to powers) 
by the use of logarithms, which transformed the operations of multiplication 
iunl Jivitiwi. Fur example, to the- simpler operation- ol addition and £tifc~1 
traction. Thus, it was often more useful to work with the logarithm of 

532 Network Analysis 

14.9 than with the number itself. We might interpret 1.173 as the "loga- 
rithmic transform" of 14.9. That is, these two numbers make up a log- 
transform pair defined by 

14.9 = 10 1173 
and 1.173 = log 14.9 

There is a unique one-to-one correspondence between the number and its 
logarithmic transform: given the number, we can find its logarithm, and, 
given the logarithm, we can calculate the corresponding number. 

We applied this concept of transformation when we analyzed the 
behavior of circuits excited by steady-state sinusoidal forcing functions. 
If we had tried to work exclusively in the time domain, we would have 
been confronted with some rather staggering sets of integrodifferential 
equations that might have chilled less stalwart hearts than ours. The 
concept of the phasor transform was introduced to ease our computational 
labors. A forcing function, v(t) = 10 cos (3t - ir/4), for example, was 
transformed into the phasor, V = 10e~' v/4 , 

10 cos (3t - f ) = ^UOe-'^X' 

Again, there is a one-to-one correspondence, on this occasion between the 
time function and its phasor transform. 

With these thoughts in mind, we are now prepared to discuss two 
integral transforms, the Fourier and Laplace transforms, which are ex- 
tremely important in the study of many types of engineering systems, 
including linear electric circuits. Up to now we have not really needed 
them, because most of our circuits, along with their forcing and response 
functions, have been rather simple. The use of relatively powerful inte- 
gral-transform techniques on them could be likened to using an electric 
locomotive to crack walnuts; we might lose sight of the meat. But now 
we have progressed to a point where our forcing functions, and perhaps 
our circuits, are getting too complicated for the tools we have developed 
so far. We want to look at forcing functions that are not periodic, and 
in later studies at (random) forcing functions or signals that are not ex- 
pressible at all as time functions. This desire is often gratified through use 
of the integral-transform methods which now burst upon us. 


Let us proceed to define the Fourier transform by first recalling the spec- 
trum of the periodic train of rectangular pulses we obtained at the end 
of Chap. 17. That was a discrete line spectrum, which is the type that 

533 f ou " er Transforms 

we must always obtain for periodic functions of time. The spectrum was 
discrete in the sense that it was not a smooth or continuous function of 
frequency; instead, it had nonzero values only at specific frequencies. 

There are many important forcing functions, however, that are not 
periodic functions of time, such as a single rectangular pulse, a step func- 
tion, a ramp function, or a rather strange type of function called the impulse 
function to be defined later in this chapter. Frequency spectra may be 
obtained for such nonperiodic functions, but they will be continuous spectra 
in which some energy, in general, may be found in any frequency interval, 
no matter how small. 

We shall develop this concept by beginning with a periodic function 
and then letting the period become infinite. Our experience with the 
periodic rectangular pulses at the end of Chap. 17 should indicate that 
the envelope will decrease in amplitude without otherwise changing shape, 
and that more and more frequency components will be found in any given 
frequency interval. In the limit we should expect an envelope of vanish- 
ingly small amplitude, filled with an infinite number of frequency compo- 
nents, separated by vanishingly small frequency intervals. The number of 
frequency components between, say, and 100 Hz becomes infinite, but 
the amplitude of each one approaches zero. At first thought, a spectrum 
of zero amplitude is a puzzling concept. We know that the line spectrum 
of a periodic forcing function shows the amplitude of each frequency 
component. But what does the zero-amplitude continuous spectrum of a 
nonperiodic forcing function signify? That question will be answered in 
the following section; now we proceed to carry out the limiting procedure 
suggested above. 

We begin with the exponential form of the Fourier series: 

f(t) = 2 •V**"*" (1) 

n—— » 


1 r T/2 


1 r T/2 
c„=^f f(t)e->™°'dt 

1 •'-J/2 


* - 2t 
u o — ~f 

We now let 

and thus, from (3), <o must become vanishingly small. We represent 
this limit by a differential 


534 N »* wo, ' k Analysis 


1 _ 

u du 

2w ~* 2w 


Finally, the frequency of any "harmonic" ruo must now correspond to the 
general frequency variable which describes the continuous spectrum. In 
other words, n must tend to infinity as co approaches zero, such that the 
product is finite: 

nw — » w (5) 

When these four limiting operations are applied to (2), we find that c„ 
must approach zero, as we had previously presumed. If we multiply each 
side of (2) by the period T and then undertake the limiting process, a 
nontrivial result is obtained: 

The right side of this expression is a function of <o (and not of t), and we 
represent it by F(/<o): 

F(/w) = J" /(*)«-*■" dt (6) 

In order to apply the limiting process to (1), we multiply and divide the 
summation by T, 

and use (4), (5), and the new quantity F(/w). In the limit, the summation 
becomes an integral, and 

/W = 2^jf F(friy'd« (7) 

Equations (6) and (7) are collectively called the Fourier transform pair. 
The function F(/<o) is the Fourier transform of f(t), and /(f) is the inverse 
Fourier transform of F(/to). 

This transform-pair relationship is most important! We should memo- 
rize it, draw arrows pointing to it, and mentally keep it on the conscious 

535 P ""*' Transform* 

level henceforth and forevermore. 1 We emphasize the importance of these 
relations by repeating and blocking them off below: 

F(p) = J* erl<"f(t) dt 

f{t) = h$ «*" F (*°) *"> 



One question is appropriate to raise at this time. For the Fourier 
transform relationships given above, can we obtain the Fourier transform 
of any arbitrarily chosen /(f)? It turns out that the answer is affirmative 
for essentially any voltage or current that we can produce. A sufficient" 
condition for the existence of F(/<o) is that 

/ |/(f)|dt<00 

This condition is not necessary, however, for some functions that do not 
meet it still have a Fourier transform; the step function is one such example. 
Furthermore, we shall see later that /(f) does not even need to be non- 
periodic in order to have a Fourier transform; the Fourier series repre- 
sentation for a periodic time function is just a special case of the more 
general Fourier transform representation. 

As in our previous work with logarithms and phasor transforms, the 
Fourier transform-pair relationship is unique. For a given /(f) there is one 
specific F(/to); and for a given F(/<o) there is one specific f(t). 

Let us use the Fourier transform to obtain the continuous spectrum 
of a single rectangular pulse. We shall select that pulse in Fig. 17-8a 
(repeated as Fig. 18- la) which occurs in the interval f < f < t + t. Thus 

po t <t<t + r 

[o t < t and t > t + t 

The Fourier transform of /(f) is found from (6): 

V e-' u ' dt 

•Future used-car dealers and politicians may forget it. 


< T 


Y*— envelope 



o *4 4 U «4 8 >o 10 >„ 12 >o 14 >o 

'o x 

o 'o 'o '0 '0 '0 

1 1 


Fig. 18-1 (a) A periodic sequence of rectangular pulses, [b] The corre- 
sponding discrete line spectrum. 

and this may be easily integrated and simplified: 

_,, . . ., sin y„WT 

■joito + T/2) 

The magnitude of F(/w) yields the continuous frequency spectrum, and it 
is obviously of the form of the sampling function. The value of F(0) is 
V t. The shape of the spectrum is identical with the broken-line curve 
of Fig. 18-lfc. A plot of |F(/u)| as a function of <o does not indicate the 
magnitude of the voltage present at any given frequency. What is it, then? 
Examination of (7) will show that F(/<o) is dimensionally "volts per unit 
frequency," a concept that may be strange to many of us. In order to 
understand this a little better, we next look into some of the properties 
of F(/<o). 

Drill Problems 

18-1 For each of the time functions given, determine F(jw) and F(j5). Let 
f(t) = outside the range of t specified, (a) I m cos 5f, — O.lw < * < O.lw; (b) 
l n cos 5t, -w <t<ir; (c) I m cos 5t, - 10w < t < lOw. 


537 Courier Transforms 

2coI 2oiI 


Ans - - « — ^sinKhru, 31.4I m ;— — ^siniru, 3.14I m 

25 - a 2 

cosO.lmoi, 0.3141 m 

1 8-2 For each of the F(/«) given, determine /(t) and/(0). Let F(/co) = outside 
the frequency range specified, (a) 1, —0.5 < w < 0.5; (b) 0.1, — 5 < u < 5; (c) 
10, -0.05 < co < 0.05. 

a„„ 0.1 sin 5t 1 sin0.5t 1 10sin0.05t 1 

•nt 2m irt 2m irt 2<n 


Our object in this section is to establish several of the mathematical prop- 
erties of the Fourier transform and, even more important, to understand 
its physical significance. We begin by using Euler's identity to replace e~ iut 
in (8a), 

F (/ W )=J f(t) cos at dt - f f f(t) sin at dt (9) 

Since f(t), cos ut, and sin ut are all real functions of time, both the integrals 
in (9) are real functions of co. Thus, by letting 

we have 

F(/co) = A(a) + jB(<o) = \F(joi)\e ieM (10) 

A(«) = J f(t) cos utdt (11) 

B(u) = - f f(t) sin ut dt (12) 

|F(/co)| = VA 2 (o>) + B\o>) (13) 

and fi( w ) = t an- 1 ^4 (14) 


Replacing co by — co shows that A(co) and |F(/co)| are both even functions 
of co, while B(co) and 0(co) are both odd functions of co. 

Now, if f(t) is an even function of t, then the integrand of (12) is an 
odd function of t, and the symmetrical limits force B(co) to be zero; thus 
the Fourier transform F(/'co) is a real, even function of co, and the phase 
function 0(co) is zero or 77 for all co. However, if f(t) is an odd function 
of t, then A(co) = 0, F(;co) is both odd and a pure imaginary function of co; 
0(u) is ±w/2. 

538 Network Analysis 

Finally, we note that the replacement of <o by -co in (9) forms the 
conjugate of F(/co). Thus, 

F(-/<o) = A(«) - ;B(u) = F*(/<o) 

and we have 

F(/«)F(-/w) = F(/co)F*(/w) = A 2 (co) + B 2 (u) = |F(/«)| 2 

With these basic mathematical properties of the Fourier transform in 
mind, we are now ready to consider its physical significance. Let us suppose 
that f(t) is either the voltage across or the current through a 1-fi resistor, 
so that f 2 ^) is the instantaneous power delivered to the 1-0 resistor by 
/(f). Integrating this power over all time, we obtain the total energy 
delivered by /(t) to the 1-fl resistor, 

W v , 

= ff 2 (t)dt (15) 

Now let us resort to a little trickery. Thinking of the integrand above as 
f(t) times itself, we replace one of those functions by (8fc>), 

Win = /"/(*) [tf «*"1W d»] * 

Since f(t) is not a function of the variable of integration co, we move it 
inside the bracketed integral, and then interchange the order of integration, 

W 10 = ^ jf [f F(We*"/(l) *] *■> 

Next we shift F(/<o) outside the inner integral, causing that integral to 
become F( — /to), 

Wia = if wpm-M du = -tf i*wi 2 *" 

Collecting these results, 

fp(t)dt = ±f\F(j<ord» (16) 

A IF, (Ml 2 

Fig. 18-2 The area of the slice [F v (/to)| 2 df is the l-£2 energy associated 
with v[t) lying in the bandwidth df. 

Equation (16) is a very useful expression known as Parseval's theorem. 2 
This theorem, along with (15), tells us that the energy associated with /(f) 
can be obtained either from an integration over all time in the time domain 
or by (1/2tt times) an integration over all frequency in the frequency 

Parseval's theorem also leads us to a greater understanding and inter- 
pretation of the meaning of the Fourier transform. Consider a voltage v(t) 
with Fourier transform F„(/<o) and 142 energy W lv , 

w„ = ±f \F v (i")\ 2 *> = if~ l F *(/<")l 2 <^ 

where the right-most equality follows from the fact that |F„(/to)| 2 is an even 
function of <o. Then, since to = 2nf, we can write 

W lr = / * |F,(M|* df = 2 j * |F,(MI 2 df 


Figure 18-2 illustrates a typical plot of |F„(/co)| 2 as a function of both <o 
and/. If we divide the frequency scale up into vanishingly small increments 
df, (17) shows us that the area of a differential slice under the |F„(jw)[ 2 
curve, having a width df, is equal to |F„(/w)| 2 df. This area is shown shaded. 
The sum of all such areas, as / ranges from minus to plus infinity, is the 
total 1-fi energy contained in v(t). Thus, \F v (ju)\ 2 is the (1-0) energy density 
or energy per unit bandwidth (J/Hz) of v(t), and, by integrating |F„(/<o)| 2 
over the appropriate frequency interval, we should be able to calculate 
that portion of the total energy lying within the given interval. 

As an example, let us assume that v(t) is the voltage forcing function 

2 Marc-Antoine Parseval-Deschenes was a rather obscure French mathematician, geographer, 
and occasional poet who published these results in 1805, 17 years before Fourier published 
his theorem. 


540 N •' wo^ ' , Analysis 

applied to the input of an ideal bandpass filter, 3 and that v (t) is the output 
voltage. For v(t) we select the one-sided [i.e., v(t) = for t < 0] exponential 

o(t) = 4e- 3t u(t) 

and let the filter passband be defined by 1 < |/| < 2. The energy in v (t) 
will therefore be equal to the energy of that part of v(t) having frequency 
components in the intervals, 1 < / < 2 and — 2 < / < — 1. We determine 
the Fourier transform of v(t), 

ao so 

F„(/<o) = 4 J e-)°<e- 3t u(t) dt = 4 J e - <3+J '" )( dt 

3 + ju 

and- then we may calculate the total 1-Q energy in the input signal either 

_ 16 /■• do> _ 8 
" i J 9 + u 2 ~ 3 J 


= J* v 2 (t)dt=ief e- 6, dt = -| J 

The total energy in t) (t), however, is smaller: 

_ l r-** Wdw 1 c*-* 16du _ 16 r** du_ 

10 ~ 2^1^ 9 + co 2 + 2tt 4 H« ! "ifl 9 + w 2 

-^^t-^t)- * 8 j 

Thus we see that an ideal bandpass filter enables us to remove energy 
from prescribed frequency ranges while still retaining the energy contained 
in other frequency ranges. The Fourier transform helps us to describe the 
filtering action quantitatively without actually evaluating v (t), although 
we shall see later that the Fourier transform can also be used to obtain 
the expression for v (t) if we wish to do so. 

3 An ideal bandpass filter is a two-port network which allows all those frequency components 
of the input signal for which a 1 < |<o| < <o 2 to pass unattenuated from the input terminals 
to the output terminals; all components having frequencies outside this so-called passband 
are completely attenuated. 

54 1 Courier Transforms 

Drill Problems 

18-3 Given i(t) = 2<r 3 l'l A, find: (a) A 4 (2); (b) B,(l); (c) |F,(jO)|. 

Atw. 0,- 0.923; 1.333 

1 8-4 Find the 1-fl energy associated with the current, i(t) = 2e~ 3 l'l A, in the 
frequency interval: (a) - 1.5 < a < 1.5; (b) -3 < u < 3; (c) -6 < a < 6 rad/s. 

Atm. 0.734; 1.092; i.278 / 


Before continuing our discussion of the Fourier transform, we need to pause 
briefly to define a new singularity function called the unit-impulse or delta 
function. We shall see that the unit-impulse function enables us to confirm 
our previous statement that periodic, as well as nonperiodic, time functions 
possess Fourier transforms. In addition, our analysis of general RLC circuits 
can be enhanced by utilization of the unit impulse. We have been avoiding 
the possibility that the voltage across a capacitor or the current through 
an inductor might change by a finite amount in zero time, for in these 
cases the capacitor current or the inductor voltage would have had to 
assume infinite values. Although this is not physically possible, it is mathe- 
matically possible. Thus, if a step voltage V u(t) is applied directly across 
an uncharged capacitor C, the time constant is zero, since R eq is zero and 
C is finite. This means that a charge CV must be established across the 
capacitor in a vanishingly small time. We might say, with more insight 
than rigor, that "infinite current flowing for zero time produces a finite 
charge" on the capacitor. This type of phenomenon can be described 
through use of the unit-impulse function. 

We shall define the unit impulse as a function of time which is zero 
when its argument, generally (t — t ), is less than zero; which is also zero 
when its argument is greater than zero; which is infinite when its argument 
is zero; and which has unit area. Mathematically, the defining statements 

8(t - t ) = t / t (18) 

and C S(t - t ) dt = 1 (19) 

where the symbol S ("curly" delta) is used to represent the unit impulse. 
In view of the functional values expressed by (18), it is apparent that the 
limits on the integral in (19) may be any values which are less than t and 



-^1 (s) 



Fig. 1 8-3 A positive and negative impulse are plotted graphically as functions 
of time. The strengths of the impulses are 4 and —3, respectively, and thus 
f(t) = 4S[t + 1 1 - 38(t). 

greater than t . In particular, we may let t and t + represent values of 
time which are arbitrarily close to t and then express (19) as 

f ° S(t- t ) dt = 1 (20) 

For the most part, we shall concern ourselves with circuits having only 
a single discontinuity, and we shall select our time scale so that the switch- 
ing operation occurs at t = 0. For this special case, the defining equations 

5(f) = t ? (21) 

and f S(i) dt = 1 (22) 

or f S(t) dt = 1 (23) 

The unit impulse may be multiplied by a constant also; this cannot, 
of course, affect (18) or (21), because the value must still be zero when 
the argument is not zero. However, multiplication of any of the integral 
expressions by a constant shows that the area under the impulse is now 
equal to the constant multiplying factor; this area is called the strength 
of the impulse. Thus, the impulse 58(t) has a strength of 5, and the impulse 
— 10S(t — 2) has a strength of — 10. If the unit impulse is multiplied by 
a function of time, then the strength of the impulse must be the value of 
that function at the time for which the impulse argument is zero. In other 
words, the strength of the impulse e~ t/2 8(t — 2) is 0.368, and the strength 
of the impulse sin (5wt + tt/4) 8(t) is 0.707. It is therefore possible to write 


543 Fourier Transforms 

the following Integrals 4 which make the same statement in mathematical 

ff(t)8(t)dt = f(0) (24) 

ff(t)8(t-t )dt = f(t ) (25) 


The graphical symbol for an impulse is shown in Fig. 18-3, where 
f(t) = 4S(t + 1) — 3S(t) is plotted as a function of time. It is customary 
to indicate the strength of the impulse in parentheses adjacent to the 
impulse. Note that no attempt should be made to indicate the strength 
of an impulse by adjusting its amplitude; each spike has infinite amplitude, 
and all impulses should be drawn with the same convenient amplitude. 
Positive and negative impulses should be drawn above and below the time 
axis, respectively. In order to avoid confusion with the ordinate, the lines 
and arrows used to form the impulses are drawn thicker than are the axes. 

We shall find it convenient to be familiar with several other inter- 
pretations of the unit impulse. We seek graphical forms which do not have 
infinite amplitudes, but which will approximate an impulse as the amplitude 
increases. Let us first consider a rectangular pulse, such as that shown in 
Fig. 18-4. The pulse width is selected as A and its amplitude as 1/A, thus 
forcing the area of the pulse to be unity, regardless of the magnitude of 
A. As A decreases, the amplitude 1/A increases, and the rectangular pulse 
becomes a better approximation to a unit impulse. The response of a circuit 
element to a unit impulse may be determined by finding its response to 
this rectangular pulse and then letting A approach zero. However, since 
the impulse response is easily found, we should also realize that this response 
may in itself be an acceptable approximation to the response produced 
by a short rectangular pulse. 

4 They are called sifting integrals because the integral sifts out a particular value of /(*). 

Fig. 18-4 A rectangular pulse of unit area which approaches a unit impulse 
as A -» 0. 


-Area = 1 

|A ±A 

Area = 1 

Fig. 18-5 A triangular pulse of unit area which approaches a unit impulse 
as A -» 0. 

A triangular pulse, sketched in Fig. 18-5, may also be used to approximate 
the unit impulse. Since we again prefer unit area, a pulse of amplitude 
1/A must possess an overall width of 2A. As A approaches zero, the 
triangular pulse approaches the unit impulse. There are many other pulse 
shapes which, in the limit, approach the unit impulse, but we shall take 
the negative exponential as our last limiting form. We first construct such 
a waveform with unit area by finding the area under the general expo- 


I Atr' /T t > 
/(*) = Ae- t/r u(t) 

Area : 

: f Ae- ,/T dt = -TAe-' /T \ = 


and we thus must set A = 1/t. The time constant will be very short, and 
we shall again use A to represent diis short time. Thus, the exponential 


approaches the unit impulse as A — * 0. This representation of the unit 
impulse indicates that the exponential decay of a current or voltage in a 
circuit approaches an impulse (but not necessarily a unit impulse) as the 
time constant is reduced. 

For our final interpretation of the unit impulse, let us try to establish 
a relationship with the unit-step function. The function shown in Fig. 18-6a 
is almost a unit step; however, A s is required for it to complete the linear 
change from zero to unit amplitude. Beneath this modified unit-step 


Fig. 18-6 (a) A modified unit-step function; the transition from zero to unity 
is linear over a A-s time interval, (b) The derivative of the modified unit step. 
As A — > 0, (a) becomes the unit step and [b) approaches the unit impulse. 

function, Fig. 18-6& shows its derivative; since the linear portion of the 
modified step rises at the rate of 1 unit every A s, the derivative must be 
a rectangular pulse of amplitude 1/A and width A. This, however, was 
the first function we considered as an approximation to the unit impulse, 
and we know that it approaches the unit impulse as A approaches zero. 
But the modified unit step approaches the unit step itself as A approaches 
zero, and we conclude that the unit impulse may be regarded as the time 
derivative of the unit-step function. 5 Mathematically, 

and conversely, 

«(*) = 


u(t) = f 8(t)dt t->0 



where the lower limit may in general be any value of t less than zero. 
Either (26) or (27) could be used as the definition of the unit impulse if 
we wished. 

5 The fact that the derivative of the unit step does not exist at the point of the discontinuity 
creates quite a skeptical attitude in many mathematicians; nevertheless, the impulse is a 
useful analytical function. 


546 Network Analysis 

. We thus see another method suggesting itself for the determination of 
the response to a unit impulse. If we can find the unit-step response, then 
the linear nature of our circuits requires the response to a unit impulse 
to be the derivative of the response to the unit step. From the opposite 
point of view, if the response to a unit impulse is known, then the integral 
of this response must be the unit-step response. 

Drill Problems 

18-5 Find the strength of the impulse defined by: (a) df/dt, where f(t) = 
2u(t - it); (b) the limit as a -» of (l/a)e- 2 \'\ /a ; (c) the limit as h -» of 
b/(x 2 + b 2 ); b>0. 

Ans. 1; 2; it 

18-6 Evaluate: (a) f Se' 2 ' 2 S(x) dx; (b) f 4(sin 2 -nt) S(t - 0.25) dt; 

5t 5(1 — sin 5wt) dr. 
_« OR 

Ans. - 1; 2; 3 


We now seek the Fourier transform of the unit impulse 8(t — t ). That 
is, we are interested in the spectral properties or frequency-domain de- 
scription of this singularity function. If we use the notation ff{ } to 
symbolize "Fourier transform of { }," then 

S{S(f-* )}= f e-i<°> 8(t - t ) 


From our earlier discussion of this type of integral, and by (25) in particular, 
we have 

5{8(t — t )} = e->"*° = cos o>t — ;' sin ut„ (28) 

This complex function of co leads to the 1-0 energy density function, 

|ff{5(* - t )}\ 2 = cos 2 ut + sin 2 ut = 1 

This remarkable result says that the (1-0) energy per unit bandwidth 
is unity at all frequencies, and that the total energy in the unit impulse 

547 Fo<"ta r Transforms 

is infinitely large. 6 No wonder, then, that we must conclude that the unit 
impulse is "impractical" in the sense that it cannot be generated in the 

Since there is a unique one-to-one correspondence between a time 
function and its Fourier transform, we can say that the inverse Fourier 
transform of e~'°" is 8(t — t ). Utilizing the symbol $F _1 { } for the inverse 
transform, we have 

ff-i{r-*"°} = S(t - t ) 

Thus, we now know that 

2^- j e + > wt e~ i ""' doi = 8(t - r ) 

even though we would fail in an attempt at the direct evaluation of this 
improper integral. Symbolically, we may write 

S(t - y » e-'"'° (29) 

where <=> indicates that the two functions constitute a Fourier transform 

Continuing with our consideration of the unit-impulse function, suppose 
that a certain time function /(f) is known to have a Fourier transform given 

F(/w) = S(u - u ) 

which is a unit impulse in the frequency domain located at cj = a) . Then 
f(t) must be 

Again using the sifting property of the unit impulse, we obtain 

6 Note, for example, from Fig. 18-4 that the total energy in the unit impulse is 
lim f (— I dt = lim (— ) = oo 

54 8 Network Analysis 

Thus we may now write 

J-e**' «* 8(<o - «„) 
or e''" ' <=* 2w5(io - <o ) (30) 

Also, by a simple sign change we obtain 

Clearly, the time function is complex in both (30) and (31), and does not 
exist in the real world of the laboratory. Time functions like cos u t, for 
example, can be produced with laboratory equipment, but a function like 
e*" ot cannot. 

However, we know that 

cos <V = V^'" ' + 1 / 2 e r ** > ' 
and it is easily seen from the definition of the Fourier transform that 

ff{/iW> + *im) = *{fi(.t)+ m) (32) 


^{coscv} = g : { 1 / 2 e'"»'} + iy{ 1 / 2 e-*'"> , } 
= ctS(io — w ) + w8(w -f- u ) 

which indicates that the frequency-domain description of cos <c t shows a 
pair of impulses, located at to = ±<o . This should not be a great surprise, 
for in our discussion of the complex-frequency plane in Sec. 13-2, we noted 
that a sinusoidal function of time was always represented by a pair of 
imaginary frequencies located at s = ±/<o . We have, therefore, 

cos u> t •» tt[8(u> + co ) + 5(<o — «„)] (33) 

Before establishing the Fourier transforms of any more time functions, 
we should understand just where we are heading, and why. Thus far we 
have determined several Fourier transform pairs. As we build up our 
knowledge of such pairs, they, in turn, can be used to obtain more pairs 
and eventually we will have a catalog of most of the familiar time functions 
encountered in circuit analysis, along with the corresponding Fourier 
transforms. Thus we will have not only the time-domain descriptions of 
such functions, but their frequency-domain descriptions as well. Then, just 
as the use of phasor transforms simplified the determination of the steady- 
state sinusoidal response, we shall find that the use of the Fourier transforms 

549 Courier Transforms 

of various forcing functions can simplify the determination of the complete 
response, both the natural and the forced components. When we extend 
our thinking to the use of the Laplace transform in the following chapter, 
we shall even be able to account for the troublesome initial conditions that 
have plagued us in the past. With these thoughts in mind, let us look at 
just a few more transform pairs with the goal of listing our findings in a 
form that will be useful for quick reference later. 

The first forcing function that we considered many chapters ago was 
a dc voltage or current. To find the Fourier transform of a constant function 
of time, f(t) = K, our first inclination might be to substitute this constant 
into the defining equation for the Fourier transform and evaluate the 
resulting integral. If we did, we would find ourselves with an indeterminate 
expression on our hands. Fortunately, however, we have already solved 
this problem, for from (31), 

We see that, if we simply let <o = 0, then the resulting transform pair 

1 » 2tt3(<o) (34) 

from which it follows that 

K <=> 2vK S(u) (35) 

and our problem is solved. The frequency spectrum of a constant function 
of time consists only of a component at <o = 0, which we knew all along. 
As another example, let us obtain the Fourier transform of a singularity 
function known as the signum function, sgn (£), defined by 



sgn« = | , (36) 

Again, if we should try to substitute this time function into the defining 
equation for the Fourier transform, we would face an indeterminate ex- 
pression upon substitution of the limits of integration. This same problem 
will arise every time we attempt to obtain the Fourier transform of a time 
function that does not approach zero as \t\ approaches infinity. Eventually, 
we will avoid this situation by defining a new kind of integral transform 
called the Laplace transform, which contains a built-in convergence factor 
that will cure many of the inconvenient ills associated with the evaluation 
of certain Fourier transforms. 

550 N «two>fc Analytis 

The signum function under consideration can be written as 

sgn (t) = lim [e- a 'u(t) - e?<u(-t)] 

a— >0 

Notice that the expression within the brackets does approach zero as \t\ 
gets very large. Using the definition of the Fourier transform, we obtain 

^{sgn (£)} = Um \j e-'^e-"' dt - J" e->»'e<" dt\ 

_ .. -/2w _ 2 
o-»o u 2 + a 2 jo 

The real component is zero since sgn(t) is an odd function of t. Thus, 

sgn (t) « f- (37) 

As a final example in this section, let us look at the familiar unit-step 
function, u(t). Making use of our work on the signum function above, we 
represent the unit step by 

«(*) = % + % sgn (t) 

and obtain the Fourier transform pair 

u(t) » Lr8(u) + i-1 (38) 

Table 18-1 presents the conclusions drawn from the examples discussed 
in this section, along with a few others that have not been detailed here. 

Drill Problems 

18-7 Find F(/2) for each function of time given: (a) 5u(t); (b) 2u(t + 0.8) — 
2u(t - 0.8); (c) e-°- 2, (cos f)u(t). 

Ans. 0.655 / -80.6° : 2.00; 2.50/ -90° 

18-8 Evaluate f(t) at t = 0.1 if £{/(<)} = : (a) 10/(3 + ju); (b) 155(<o - 4) + 

An*. 4.40; 7.41; 8.00 

158( U + 4); (c) ^^ - f! 

551 Fourier Transfoims 
Table 18-1 Seme familiar Fourier transform pairs 





S(t - g 

${f(t)} = f(H 




2ir6(to — to ) 



cos w f 

7r[6(to + co ) + 5(w - w )] 

J^ 1 

-«„ w, 




♦ (2ir) 





ttS(u) + ■ 

? <0 


a + )'« 

> « 


e "' cos Wjt • u(t) 

a + ju 

(a + jaf + u d 2 


-«J «. 





u(t + y 2 r) - u(« - %r) 

2 2 


T T 

552 Nelworlt Analysis 


In Sec. 18-2 we remarked that we would be able to show that even periodic 
time functions possess Fourier transforms. Since a promise made is a debt 
unpaid, let us now establish this fact on a rigorous basis. Consider a periodic 
time function /(f) with period T and Fourier series expansion, as outlined 

by (1), (2), and (3), 

f(t) = £ c n e»«°< (1) 


^n=~f /2 f{t)e- in ' i "' l dt (2) 

and Wo = ^ (3) 

Bearing in mind that the Fourier transform of a sum is just the sum of 
the transforms of the terms in the sum, and that c„ is not a function of 
time, we can write 

Substituting the transform of e'"" ' given in (30), we have 

/(*) «2 ff I c„5(« - no> ) (39) 

This shows that f(t) has a discrete spectrum consisting of impulses located 
at points on the <o axis given by to = ruc , n = . . . , —2, — 1, 0, 1, . . . . 
The strength of each impulse is 2w times the value of the corresponding 
Fourier coefficient appearing in the complex form of the Fourier series 
expansion for f(t). 

Now, if the expression for the transform pair shown in (39) is valid, 
then the inverse Fourier transform of the right side should be f(t). This 
inverse transform can be written as 

ff-»{F(M} = i f e M [a* J "»«(<•> - ™o)] *» = /(*) 

553 Courier Transform* 

Since the exponential term does not contain the index of summation n, 
we can interchange the order of the integration and summation operations, 

ff-i{F(/(o)} = 2 / c„e*" ( S(<o - ruo ) du I f(t) 

Because it is not a function of the variable of integration to, c„ can be treated 
as a constant. Then, using the sifting property of the impulse, we obtain 

SF-i{F(/<o)} = 2 c„e*""°' =f(t) 

which is exacdy the same as (1), the complex Fourier series expansion for 
f(t). The question marks in the preceding equations can now be removed, 
and the existence of the Fourier transform for a periodic time function 
is established. This should come as no great surprise, however. In the last 
section we evaluated the Fourier transform of a cosine function, which 
is certainly periodic, although we made no direct reference to its peri- 
odicity. However, we did use a backhanded approach in getting the 
transform. But now we have a mathematical tool by which the transform 
can be obtained more directly. To demonstrate this procedure, consider 
f(t) = cos u t once more. First we evaluate the Fourier coefficients c n , 

c " = Yf2 cos " ote ~ in "°' dt= {o 

% n=±l 



ff{/(t)} = 2* ^ c„S(<o - mo ) 

This expression only has values that are nonzero when n = ±1, and it 
follows, therefore, that the entire summation reduces to 

SF{cos <o f} = ir[S(oi — io ) + S(u + w )] 

which is precisely the expression that we obtained before. What a relief ! 

Drill Problem 

1 8-9 Determine the Fourier transform for: (a) 10 cos 5t; (b) 10 sin 5t; (c) 

10 cos (5* + ir/3). 

Ans. 10ir[S(u + 5) + S(u - 5)]; jlOTr[8{a + 5) - 6(a - 5)]; 
lOale-^'Shlu + 5) + ^ /3 S(o> - 5)] 

554 Network Analysis 


Before continuing our discussion of the Fourier transform, let us note again 
where all this is leading. Our goal is a technique for simplifying problems 
in linear circuit analysis which involve the determination of explicit ex- 
pressions for response functions caused by the application of one or more 
forcing functions. We accomplish this by utilizing a mathematical quantity 
called the system function or transfer function of the circuit. It turns out 
that this system function is the Fourier transform of the unit-impulse 
response of the circuit. The specific analytical technique that will be used 
requires the evaluation of the Fourier transform of the forcing function, 
the multiplication of this transform by the system function to obtain the 
transform of the response function, and then the in verse- transform operation 
to obtain the response function. By these means some relatively compli- 
cated integral expressions will be reduced to simple functions of to, and 
the mathematical operations of integration and differentiation will be 
replaced by the simpler operations of algebraic multiplication and division. 
With these remarks in mind, let us now proceed to examine the unit-impulse 
response of a circuit and eventually establish its relation to the system 
function. Then we can look at some specific analysis problems. 

Consider an electric network N without initial stored energy to which 
a forcing function x(t) is applied. At some point in this circuit, a response 
function y(t) is present. We show this in block diagram form in Fig. 18-7o 
along with general sketches of typical time functions. The forcing function 
is arbitrarily shown to exist only over the interval a < t < b. Thus, y(t) 
can exist only for t > a. The question that we now wish to answer is this: 
if we know the form of x(t), then how is y(t) described? To answer this 
question, it is obvious that we need to know something about N. Suppose, 
therefore, that our knowledge of N is the way it responds when the forcing 
function is a unit impulse. That is, we are assuming that we know h(i), 
the response function resulting from a unit impulse being supplied as the 
forcing function at t = 0, as shown in Fig. 18-7b. The function h(i) is 
commonly called the unit-impulse response function or the impulse re- 
sponse. This is a very important descriptive property for an electric circuit. 
Instead of applying the unit impulse at time t = 0, suppose that it were 
applied at time t — A. It is evident that the only change in the output 
would be a time delay. Thus, the output becomes h(t — A) when the input 
is S(t — A), as shown in Fig. 18-7c. Next, suppose that the input impulse 
were to have some strength other than unity. Specifically, let the strength 
of the impulse be numerically equal to the value of x(t) when t = A. This 
value x(\) is a constant; we know that the multiplication of a single forcing 
function in a linear circuit by a constant simply causes the response to 
change proportionately. Thus, if the input is changed to x(\)S(t — A), then 
the response becomes x(\)h(t — A), as shown in Fig. 18-7d. Now let us 


*<(>*= id) 












/*i(X)«(l-X) d\ 

f~x(\)h(t-\) d\ 



fx(\)h(t-\) d\ = y(t) 


Fig. 18-7 A conceptual development of the convolution integral, 

ym = /;«, *M>>(t - X) dx. 

sum this latest input over all possible values of X and use the result as a 
forcing function for N. Linearity decrees that the output must be equal 
to the sum of the responses resulting from the use of all possible values 
of A. Loosely speaking, the integral of the input produces the integral of 
the output, as shown in Fig. 18-7e. But what is the input now? Using the 
sifting property of the unit impulse, we see that the input is simply x(t), 
the original input. 

Our question is now answered. When x(t), the input to N, is known, 
and when h(t), the impulse response of iV, is known, then y(t), the output 
or response function, is expressed by 

y(t) = J x(\)h{t -\)d\ 


as shown in Fig. 18-7/. This important relationship is known far and wide 
as the convolution integral. In words, this last equation states that "the 


556 Ne,wo >* Analysis 

output is equal to the input convolved with the impulse response." It is 
often abbreviated by means of 

y(t) = x(t) - h(t) (41) 

where the asterisk is read "convolved with." 

Equation (40) sometimes appears in a slightly different but equivalent 
form. If we let z — t — A, the expression for y(t) becomes 

y(t) = f -x(t - z)h(z)dz = f x(t — z)h(z) dz 

and, since the symbol that we use for the variable of integration is un- 
important, we can write 

y{t) = x(i) « h(t) = J x(z)Mt - z)dz = j x(t - z)h(z) dz (42) 

These two forms of the convolution integral are worth memorizing. 

The result that we have in (42) is very general. It applies to any linear 
system. However, we are interested in physically realizable systems, those 
that do exist or could exist, and such systems have a property that modifies 
the convolution integral slightly. That is, the response of the system cannot 
begin before the forcing function is applied. In particular, h(t) is the 
response of the system resulting from the application of a unit impulse 
at t = 0. Therefore, h(t) cannot exist for t < 0. It follows that, in the 
second integral of (42), the integrand is zero when z < 0; in the first 
integral, the integrand is zero when i — z is negative or when z > t. 
Therefore, for realizable systems the limits of integration change in the 
convolution integrals: 

r' r' 

y(t) = x(i) * h{t) = / x(z)Mt - z)dz= I x(t - z)h(z) dz (43) 

•'-=0 ••'o 

Equations (42) and (43) are both valid, but the latter is more specific when 
we are speaking of realizable linear systems. 

Before discussing the significance of the impulse response of a circuit 
any further, let us consider a numerical example which will give us some 
insight into just how the convolution integral can be evaluated. Although 
the expression itself is simple enough, the evaluation is sometimes trouble- 
some, especially with regard to the values used as the limits of integration. 

Suppose that the input is a rectangular voltage pulse that starts at t = 0, 
has a duration of 1 s, and is 1 V in amplitude, 

X(t) = Uj(f) = u(t) - u(t - 1) 

557 f°"" et Transform* 

Suppose also that the impulse response of this circuit is known to be an 
exponential function of the form: 7 

hit) = 2e-'u(t) 

We wish to evaluate the output voltage v (t), and we can write the answer 
immediately in integral from, 

y(t) = v (t) = Vt(t) ♦ h(t) = I v t (t - z)h(z) dz 
J o 

= f [u(t - z) - u(t-z- l)][2e- z u(z)] dz 

Obtaining this expression for v (t) was simple enough, but the presence 
of the many unit-step functions tends to make its evaluation confusing. 
Careful attention must be paid to determine those portions of the range 
of integration in which the integrand is zero. Let us first use some graphical 
assistance to help us understand what it says. We first draw some horizontal 
z axes lined up one above the other, as shown in Fig. 18-8, We know what 
«((£) looks like, so we know what v^z) looks like also; this is plotted as 
Fig. 18-8a. The function v t ( — z) is simply v^z) run backwards with respect 
to z, or rotated about the ordinate axis; it is shown in Fig. 18-8b. Next 
we wish to represent v^t — z), which is v t ( —z) after it is shifted to the 
right by an amount z — t as shown in Fig. 18-8c. On the next z axis in 
Fig. 18-8d, the hypothetical impulse response is plotted. Finally, we 
multiply the two functions v t (t — z) and h(z). The result is shown in Fig. 
18-8e. Since h(z) does not exist prior to t = and v t (t — z) does not exist 
for z > t, notice that the product of these two functions has nonzero values 
only in the interval < z < t for the case shown where t < 1 ; when t > 1, 
then the nonzero values for the product are obtained in the interval, 
(t — 1) < z < t. The area under the product curve (shown shaded in the 
figure) is numerically equal to the value of v corresponding to the specific 
value of t selected in Fig. 18-8c. As t increases from zero to unity, the 
area under the product curve continues to rise, and thus v (i) continues 
to rise. But as t increases beyond t = 1, the area under the product curve, 
which is equal to v (t), starts decreasing and approaches zero. For * < 0, 
the curves representing v t (t ^- z) and h(z) do not overlap at all, so the area 
under the product curve is obviously zero. Now let us use these graphical 
concepts to obtain an explicit expression for v (t). 

For values of t that lie between zero and unity, we must integrate from 

7 A description of one possible circuit to which this impulse response might apply is developed 
in Prob. 27. 

Oj U> 








1 2 3 

Fig. 18-8 Graphical concepts in evaluating a convolution integral. 

z — to z — t; for values of t that exceed unity, the range of integration 
is t — 1 < z < t. Thus, we may write 



f 2e"* dz = 2(1 - e-<) < t < 1 

f 2e~ z dz = 2(e - l)e"' < > 1 

This function is shown plotted versus the time variable t in Fig. 18-8/, and 
our problem is completed. There is a great deal of information and tech- 


559 Fouriar Transforms 

nique wrapped up in this one example problem. The drill problems below 
offer an opportunity to make sure that the procedure is understood suffi- 
ciently well to make it worthwhile passing on to new material. 

Drill Problems 

18-10 Given the impulse response for a network N, h(t) = u(f) — u(t — 1), and 
the input signal, v t = 2e~'u(t) V, determine v„(t) at t = : (a) —0.5; (b) 0.5; (c) 
1.5 s. 

Am. 0; 0.767; 0.787 V 

18-11 When the current source, i s = S(t) A, is applied to a certain network, 
the output voltage is 5[u(t) - u(t — 4)] V. If the source,!, = 2t[u(t) — u(t — 3)] A, 
is applied, find the output voltage at t = : (a) 2; (b) 3.62; (c) 5 s. 

Arts. 20; 40; 45 V 


In the previous section the problem of determining the output of a physical 
system in terms of the input and the impulse response was solved by using 
the convolution integral and working entirely in the time domain. The 
input, the output, and the impulse response are all time functions. Now 
let us see whether some analytical simplification can be wrought by working 
with frequency-domain descriptions of these three functions. 

To do this we examine the Fourier transform of the system output, 
utilizing the basic definition of the Fourier transform and the output 
expressed by the convolution integral (42), 

*{»„«} = F.f/u) = J e-*°> If v,(t - z)h(z) dz\ dt 

where we again assume no initial energy storage. At first glance this 
expression may seem rather formidable, but it can be reduced to a result 
that is surprisingly simple. We may move the exponential term inside the 
inner integral because it does not contain the variable of integration z. 
Next we reverse the order of integration, obtaining 

F„(M = / / e-i"'v l (t-z)h(z)dtdz 
Since it is not a function of t, we can extract h(z) from the inner integral 

560 Network Analysis 

and simplify the integration with respect to t by a change of variable, 
t — z = x, 

F (jo>) = J h(z) J V* o(l+ ' r> e J (x) dxdz 

= f e- iu *h(z)J e-^'v^dxdz 

But now the sum is starting to break through, for the inner integral is merely 
the Fourier transform of v t (t). Furthermore, it contains no z terms and 
can be treated as a constant in any integration involving z. Thus, we can 
move this transform, F^/to), completely outside all the integral signs, 

F.(H = F,(M/"« r *"*(a)'b 


Finally, the remaining integral exhibits our old friend once more, another 
Fourier transform! This one is the Fourier transform of the impulse re- 
sponse, which we shall designate by the notation H(/co). Therefore, all our 
work has boiled down to the simple result: 

F„(/<o) = F f (/<o)H(p) = F^i^ihit)} (44) 

This is another important result; it defines for us the meaning of the system 
function H(/<o). The system function is the ratio of the Fourier transform 
of the response function to the Fourier transform of the forcing function. 
Moreover, the system function and the impulse response comprise a Fourier 
transform pair: 

h(t) «» H(/<o) (45) 

The development in the preceding paragraph also serves to prove the 
general statement that the Fourier transform of the convolution of two 
time functions is the product of their Fourier transforms, 

S{/W*g(*)}=F,(/<o)F t (/<o) (46) 

To recapitulate, if we know the Fourier transforms of the forcing 
function and the impulse response, then the Fourier transform of the 
response function can be obtained as their product. The result is a descrip- 
tion of the response function in the frequency domain; if we wish to do 
so, we can obtain the time-domain description of the response function 
by taking the inverse Fourier transform. Thus we see that the process of 

56 1 Fourier Transforms 

convolution in the time domain has been reduced to the relatively simple 
operation of multiplication in the frequency domain. This is one fact that 
makes the use of integral transforms so attractive. 

The foregoing comments might make us wonder why we would ever 
choose to work in the time domain, but we must always remember that 
we seldom get something for nothing. A poet once said, "Our sincerest 
laughter, with some pain is fraught." 8 The pain herein is the occasional 
difficulty in obtaining the inverse Fourier transform of a response function, 
for reasons of mathematical complexity. On the other hand, a modern 
digital computer can convolve two time functions with magnificent celer- 
ity. For that matter, it can also obtain an FFT (fast Fourier transform) 9 
quite rapidly. Consequently there is no clear-cut advantage between 
working in the time domain or the frequency domain. A decision must 
be made each time a new problem arises; it should be based on the given 
information available and on the computational facilities at hand. 

Now let us attempt a frequency-domain analysis of the problem that 
we worked in the preceding section with the convolution integral. Re- 
calling that we had a forcing function of the form 

v t (t) = u(t) - u(t - 1) 

and a unit-impulse response defined by 

h(t) = 2e~ t u(t) 

we first obtain the corresponding Fourier transforms. The forcing function 
is the difference between two unit-step functions. These two functions are 
identical, except that one is initiated 1 s after the other. We shall evaluate 
that the response due to u(t) and the response due to u(t — 1) will be the 
same, but delayed in time by 1 s. The difference between these two partial 
responses will be the total response due to v t (t). 

The Fourier transform of u(t) was obtained in Sec. 18-5, 

${u(t)} = wSta) -(- ± 

The system function is obtained by taking the Fourier transform of h(t), 
listed in Table 18-1, 

3{h(t)} = H(;<o) = SF{2e-'tt(<)} = — f^- 

1 + ]03 

8 A cultural message from P. B. Shelley, "To a Skylark," 1821. 

9 The fast Fourier transform is a type of discrete Fourier transform, which is a numerical 
approximation to the (continuous) Fourier transform we have been considering. Many 
references concerning it are given in G. D. Bergland, A Guided Tour of the Fast Fourier 
Transform, IEEE Spectrum, vol. 6, no. 7, pp. 41-52, July 1969. 

562 Network Analysis 

The inverse transform of the product of these two functions yields that 
component of v (t) caused by tt(t), 

, . _ . (SM(u) 2 i 

Using the sifting property of the unit impulse, the inverse transform of 
the first term is just a constant equal to unity. After breaking the second 
term up into partial fractions, 

^i + s-^-rf-} 

the inverse transforms are taken from Table 18-1 once more: 

v 01 (f) = 1 + sgn (t) - 2e~'u(t) 
= 2u(t) - 2e-'u(t) 
= 2(1 - e-')«(*) 

It follows that v o2 (t), the component of v (t) produced by u(t — 1), is 

v o2 (t) = 2(1 - e-o-Xf - 1) 

c„« = t) 01 (t) + v o2 (t) 

= 2(1 - e-')u(t) - 2(1 - e-' +1 )u(t - 1) 

The discontinuities at t = and t — 1 dictate a separation into three time 


v (t) = 2(1 - e->) < t < 1 

,2(e-l)e-' f>l 

This is the same result we obtained by working this problem with the 
convolution integral in the time domain. 

It appears that some ease of solution is realized by working this partic- 
ular problem in the frequency domain rather than in the time domain. 
We are able to trade a relatively complicated time-domain integration for 
a simple multiplication of two Fourier transforms in the frequency domain, 
and (this is a most noteworthy point) we did not have to pay the price 
of having a difficult Fourier transform to invert in determining v (t). 

563 Fewtor Transforms 

Drill Problems 

1 8-1 2 If h(t) = 2e- 3 'u(t) and v { (t) = 3 e - 2t u(t), first find H(/w), V^/w), and V„(ju) = 
Vj(/(<))H(p), and then evaluate v (t) at t = : (a) 0.5; (b) 1.0; (c) 1.5 s. 

Arw. 0.232; 0.513; 0.869 V 

18-13 Use frequency-domain methods to find the time-domain response of a 
network having a system function, j2oi/(i + j2u), if the input is: (a) a unit im- 
pulse; (b) a unit-step function; (c) cos t. 

Am. e- t/2 u(t); 8(t) - 0.5e-' /2 u(t); 0.8 cost - 0.4 sin t 


In this section we shall try to connect several aspects of the Fourier 
transform with work we have completed in earlier chapters. 

Given a general linear two-port network N without any initial energy 
storage, we assume sinusoidal forcing and response functions, arbitrarily 
assumed to be voltages, as shown in Fig. 18-9. We let the input voltage 
be simply A cos ((c x t + 6), and the output can be described in general terms 
as £>„(£) = B cos (w x t + <#>), where the amplitude B and phase angle <#> are 
functions of u r In phasor form, we can write the forcing and response 
functions as V t — Ae? 9 and V = Be'*. The ratio of the phasor response 
to the phasor forcing function is a complex number that is a function 
of u x , 

y t = gk) = !•**-« 

where B/A is the amplitude of G and <t> — 6 is its phase angle. This function 
G(u x ) is the frequency-response function for N, and it could be obtained 
in the laboratory by varying u x over a large range of values, and measuring 
the amplitude B/A and phase <£ — 8 for each value of oi x . If we would 
then plot each of these parameters as a function of frequency, the resultant 
pair of curves would completely describe the frequency-response function. 
Now let us hold these comments in the backs of our minds for a moment 
as we consider a slightly different aspect of the same analysis problem. 

Fig. 18-9 Sinusoidal analysis can be used to determine the transfer function. 
fUjaJ = {B/A)e M ''\ where B and <f> are functions of u>,. 

i>j (() = A cos(ai !r t+S) f/ e (t) = B cos(oi x t+<j>) 

564 Network Analysis 

For the circuit with sinusoidal input and output shown in Fig. 18-9, 
what is the system function H(/to)? To answer this question, we begin with 
the definition of H(/co) as the ratio of the Fourier transforms of the output 
and the input. Both of these time functions involve the functional form, 
cos (co x t + /3), whose Fourier transform we have not evaluated as yet, 
although we can handle cos u x t. The transform we need is 

SFfcos (a x t + /?)} = J e~*" cos (a x t + 0) dt 
If we make the substitution, u> x t + /S = w x t, then 

${cos (u x t + /?)} = f e -J*r+u>fi/** cos UxT dr 
_ ^H^'^{ COSUx t} 
= 7 re , '" /J/ "'[8(<o - u x ) + S(u + w,)] 
This is a new Fourier transform pair, 

cos (o>J + /?)*=> ■ne>""'"'{6(<* - a z ) + 8(o> + coj] (47) 

which we can now use to evaluate the desired system function, 

5{B cos (a.t + »)} 
(M ~ if [A cos (to,* + B)} 

_ ■KBe'^ /u '[S(w - a x ) + 8(oi 4- u x )] 
~ ■nAel" s/ ">[8(o> - u x ) + S(u + u x )] 

~ A e 

Now we recall the expression for G(u x ), 

where B and <J> were evaluated at <o = w x , and we see that evaluating 

H(/to) at co = a x gives 

H(/coJ = G(coJ = £«**-« 

565 ^ our < or Transforms 

Since there is nothing special about the x subscript, we conclude that the 
system function and the frequency-response function are identical: 

H(/<o) = G(w) (48) 

The fact that one argument is &> while the other is indicated by fu is 
immaterial and arbitrary; the / merely makes possible a more direct com- 
parison between the Fourier and Laplace transforms. 

Equation (48) represents a direct connection between Fourier transform 
techniques and sinusoidal steady-state analysis. Our previous work on 
steady-state sinusoidal analysis using phasors was but a special case of the 
more general techniques of Fourier transform analysis. It was "special" 
in the sense that the inputs and outputs were sinusoids, whereas the use 
of Fourier transforms and system functions enables us to handle non- 
sinusoidal forcing functions and responses. 

As an example of the application of these profound generalities, let us 
look at the simple RL series circuit shown in Fig. 18- 10a. We seek the 
voltage across the inductor when the input voltage is a simple exponentially 
decaying pulse. We need the system function; but it is not necessary to 
apply an impulse, find the impulse response, and then determine its inverse 
transform. Instead we use (48) to obtain the system function H(/to) by 
assuming that the input and output voltages are both sinusoids described 
by their corresponding phasors, as shown in Fig. 18-10fo. Using voltage 
division, we have 

wo.* - v ° - P" 

The transform of the forcing function is 

5{v t (t)} = - - 5 

3 + ju 

Fig. 18-10 (a) The response v [t) caused by v^t) is desired, (b) The system 
function H(;a>) may be determined by sinusoidal steady-state analysis: 
H(/ W ) = V./V,. 

566 Natwotfc Anoiytii 

and thus the transform of v„(t) is given as 

9{vM = H(/<o)ST{ Cl (f)} 
j2u 5 

4 + /2w 3 + joi 
15 10 

3 + ;w 2 + /<o 

where the partial fractions appearing in the last step help to determine 
the inverse Fourier transform 


= 15e- 3, u(t) - 10e- 2 'u(t) 
= 5(3e- 3 ' - 2e- 2t )u(t) 

Our problem is completed without fuss, convolution, or differential equa- 

Returning again to (48), the identity between the system function H(/w) 
and the sinusoidal steady-state frequency-response function G(oi), we may 
now consider the system function as the ratio of the output phasor to the 
input phasor. Suppose that we hold the input-phasor amplitude at unity 
and the phase angle at zero. Then the output phasor is H(/w). Under these 
conditions, if we record the output amplitude and phase as functions of 
to, for all <o, we have recorded the system function H(/to) as a function of 
to, for all to. We thus have examined the system response under the condi- 
tion that an infinite number of sinusoids, all with unity amplitude and zero 
phase, were successively applied at the input. Now suppose that our input 
is a single unit impulse and look at the impulse response h(t). Is the 
information we examine really any different from that we just obtained? 
The Fourier transform of the unit impulse is a constant equal to unity, 
indicating that all frequency components are present, all with the same 
magnitude, and all with zero phase. Our system response is the sum of the 
responses to all these components. The result might be viewed at the 
output on a cathode-ray oscilloscope. It is evident that the system function 
and the impulse-response function contain equivalent information regarding 
the response of the system. 

We therefore have two different methods of describing the response 
of a system to a general forcing function; one is a time-domain description, 
and the other a frequency-domain description. Working in the time domain, 
we convolve the forcing function with the impulse response of the system 
to obtain the response function. As we saw when we first considered 

567 F 0" rl » r Tranrionm 

convolution, this procedure may be interpreted by thinking of the input 
as a continuum of impulses of different strengths and times of application; 
the output which results is a continuum of impulse responses. 

In the frequency domain, however, we determine the response by 
multiplying the Fourier transform of the forcing function by the system 
function. In this case we interpret the transform of the forcing functiott 
as a frequency spectrum, or a continuum of sinusoids. Multiplying this by 
the system function, we obtain the response function, also as a continuum 
of sinusoids. 

Whether we choose to think of the output as a continuum of impulse 
responses or as a continuum of sinusoidal responses, the linearity of the 
network and the superposition principle enable us to determine the total 
output as a time function by summing over all frequencies (the inverse 
Fourier transform), or as a frequency function by summing over all time 
(the Fourier transform). 

Unfortunately, both of these techniques have some difficulties or limita- 
tions associated with their use. In using convolution, the integral itself can 
often be rather difficult to evaluate when complicated forcing functions 
or impulse response functions are present. Furthermore, from the experi- 
mental point of view, we cannot really measure the impulse response of 
a system because we cannot actually generate an impulse. Even if we 
approximate the impulse by a short high-amplitude pulse, we should 
probably drive our system into saturation and out of its linear operating 

With regard to the frequency domain, we encounter one absolute 
limitation in that we may easily hypothesize forcing functions that we 
would like to apply theoretically that do not possess Fourier transforms. 
Moreover, if we wish to find the time-domain description of the response 
function, we must evaluate an inverse Fourier transform, and some of these 
inversions can be extremely difficult. 

Finally, neither of these techniques offers a very convenient method 
of handling initial conditions. 

The greatest benefits derived from the use of the Fourier transform arise 
through the abundance of useful information it provides about the spectral 
properties of a signal, particularly the energy or power per unit bandwidth. 

Most of the difficulties and limitations associated with the Fourier 
transform are overcome with the use of the Laplace transform. We shall 
see that it is defined in such a way that there is a built-in convergence 
factor that enables transforms to be determined for a much wider range 
of input time functions than the Fourier transform can accommodate. 
Moreover, we shall find that initial conditions may be handled in a manner 
that may make us wonder why this marvelous technique was not introduced 
before the last chapter. Finally, the spectral information that is so readily 

568 N***™' 11 Analysis 

available in the Fourier transform can also be obtained from the Laplace 
transform, at least for most of the time functions that arise in real engineer- 
ing problems. 

Well, why has this all been withheld until now? The best answer is 
probably because these powerful techniques can overcomplicate the 
solution of simple problems and tend to obscure the physical interpretation 
of the performance of the simpler networks. For example, if we are 
interested only in the forced response, then there is little point in using 
the Laplace transform and obtaining both the forced and natural response 
after laboring through a difficult inverse transform operation. 

So much for generalities; on to Laplace. 

Drill Problem 

18-14 Using Fourier transform methods, find v c in the circuit of Fig. 18-11 at 

t = 0.5 s if i s = : (a) 8(t); (b) u(t); (c) u(t) - u(t - 0.4). 

Ans. 148; 214; 215 V 

*^A 1 

1000 *iF;fc "c 

Fig. 18-11 See Drill Prob. 18-14. 


□ 1 Find the Fourier transforms for the waveforms illustrated in Fig. 18-12. 

Fig. 18-12 See Prob. 1. 







Sine curve 


569 Courier Transforms 

□ 2 Given the function, /(f) = sin 2irt, < t < %, and f(i) = for t > % and 
f < — %, define f(t) for — % < t < so that: (a) /(t) is an odd function and 
determine F(/&>); (fc) fit) is an even function and determine F(/<o). 

□ 3 Determine the Fourier transform of the waveform shown in Fig. 18-13. 


-2-1 12 

Fig. 18-13 See Prob. 3. 

□ 4 For each continuous frequency spectrum given, determine f(t): (a) F(/ai) = 
e-i"l; (b) F(/«) = e-Mu(|w| - 1); (c) F(ju) = e -M„(l - |<o|); (d) F(p) = e-"tt(«). 

D 5 If F(/«) is both a real and an even function of oi: (a) show that /(() =t 

(1/w) J F(/<o) cos uf dw. If F(/w) = l/|fa>| for 1 < |u| < 2 and is zero elsewhere: 

(b) evaluate /(0); (c) use graphical or numerical methods to approximate /(w/2). 

□ 6 Find the total 1-0 energy associated with the voltage: (a) Ae~ b 'u(t); (b) Ae'^'K 

□ 7 Given the current pulse, i(t) = te~ b 'u(t): (a) find the total 1-U energy associated 
with this waveform by two different methods, (b) What fraction of this energy 
is present in the frequency band from — b to b rad/s? 

D 8 (a) Let a > and show that the Fourier transform of f(t) = e _a, (cos u d t)u(t) 
is (a + joi)/[(a + ;'w) 2 + o) d 2 ]- Find the total 1-fl energy associated with 
e~'(cos t)u(t) by using a: (b) time-domain integration; (c) frequency-domain inte- 

gration. I Hint: J [(x 2 + l)/(x 4 + 4)] dx = 3tt/8.] 

□ 9 An ideal source, i s — S(t) mA, is applied to a 2-juF capacitor and a 50042 
resistor in parallel, as illustrated in Fig. 18-14a. Find: (a) i K (t); (b) i c (t); (c) v(t). 
Determine the total energy: (d) dissipated in the resistor; (e) provided by the 

Fig. 18-14 (a) See Prob. 9. (fe) See Prob. 10. 


2 fiFsfc « 

570 Network Analysis 

□ 10 With reference to the circuit shown in Fig. 18-14&, let t, = 0.1u(f) A and 
find: (a) v K (t); (b) v L (t); (c) v,(t). 

□ 11 (a) In Fig. 18-15, let v^t) = 8(t) V, and find v 2 (t). (b) Let Cl (t) = u(t) V, and 
find v 2 (t). (c) Show that the forcing function in part (a) is the derivative of the 
forcing function in (b), and that the response in (a) is the derivative of the response 
in (b). 

150 n 3H 

o — VVVi — • TJl'>- 


o,(0 300 n< zoo a< °2<" 

o 1 1 <> 

Fig. 18-15 See Prob. 11. 

□ 12 A rectangular voltage pulse, v(t) = 10J; \u(t) — u\t — j-)\ V, is applied in 

series with a 100-fjF capacitor and a 20-kQ resistor. Find the capacitor voltage 
at t = 1 if: (a) fe = 1; (fc) fc = 10; (c) fc = 100; (d) in the limit as k -> oo. 

D 13 ' Find the Fourier transform of each of the following functions of time: (a) 

e- (1+t2) 5(*); (b) [sgn (r)][u(t + 1) - tt(f - 1)]; (c) 10cos 2 4f. 

D 14 Use the definition of the Fourier transform to prove the following results: 

(a) 5{/(t - t )} = r*»9{f(t)h (b) Z{df(t)/dt) = /«ff {/(*)}; (c) ff{/(fa)} = 
(l/|fc|)F(/«/fc), where S{/«} = F(/<o); (d) *{/(-<)} = F(-/<o). 

D 15 Prove the following Fourier transform pairs: (a) e'u( — t) <=> 1/(1 — ju); (b) 
e-l'l «* 2/(1 -I- <o 2 ); (c) e-«'(sin «„*)«!(») ** o> d /[(a + ;<o) 2 + «/]. 

D 16 Find and sketch as a function of time the inverse Fourier transform corre- 
sponding to F(/a>) = : (a) /w/(l + co 2 ); (b) 1/[(1 + ja)(2 + ja)]. 

a 17 Find/(«) if 5F{/(*)} = : (a) 1/(1 - w 2 + fa); (b) 1/{(1 + /u)(2 + ;«)(3 + Jw)]. 

D 18 (a) Given f{t) <=» F(/u), show that tf(t) <z* j dF(ju)/du. (b) Find 
SF"i{l/(l + M 2 }. 

□ 19 Find the Fourier transform of the periodic waveform shown in Fig.: (a) 
18-16a; (b) 18-16b. 


□ 20 Given F(/<o) = 10vS(w) - jlO 2 (Vn)[S(« -I- 20»m) - S(u - 20™)], find 

D 21 Convolve «(t) with fc(t) for these pairs of functions: (a) *(*) = h(t) = «(t) — 
«(* - 1); (b) x(t) = 2e'u(t), h(t) = (cos «)«(«)• 








J-> t 

Fig. 18-16 See Prob. 19. 

□ 22 (a) Sketch the waveshape versus t which results when the two functions shown 
in Fig. 18-17a are convolved, (b) Repeat for Fig. 18-17fo. 















-1 - 

1\ /2 

Sine curve 

Hg. 18-17 See Probs. 22 and 23. 

D 23 Show that both forms of the convolution integral given by (42) in Sec. 18-7 
lead to the same result for the time functions shown in Fig. 18-17a. 

D 24 If y(t) = f(t) • git), find y(t) for F(;<o) = 1/(1 + u 2 ) and G(ju) = 2 + S(u) by 
convolution in the: (a) frequency domain; (b) time domain. 


572 Network Analysis 

a 25 

If Y(ju) = F(/<o)H(/w), find y(t) for F(/«) = H(/a>) = 1/(1 + « 2 ). 

D 26 Find the system function, H(/<o) = V^/toyi^/a)), and impulse response of u 
one-port network if the input voltage, v^i) = 100 cos oi t V, produces the input 
current, !,(/«) = 100ir[S(u + <o ) + 5(« - w )](l - //2u). 

□ 27 In Sec. 18-7 the impulse response, h(t) = 2e~'u(f), was hypothesized. In order 
to develop one network which has such a response: (a) determine H(/<o) = 
V o(/")/ V i(/ w )- (b) Either by inspecting h(t) or H(/u), note that the network has 
a single energy storage element. Arbitrarily selecting an RC circuit with R = 1 fi, 
C = 1 F, to provide the necessary time constant, determine the form of the circuit 
to give y 2 fc(t) or l / 2 H(/<o). (c) Place an ideal-voltage amplifier in cascade with the 
network to provide the proper multiplicative constant. What is the gain of the 

D 28 Find v (t) in the LC circuit shown in Fig. 18-18 if e,(t) = S(t). (Hint: See 
Prob. 15c.) 

- r SSV^- 

=F »„(«) 

Fig. 18-18 See Prob. 28. 

D 29 Find („(() in the circuit shown in Fig. 18-19 if c s (t) = : (a) &(t) V; (b) u{t) V; 
(c) e-'u(t) V. 

Fig. 18-19 See Prob. 29. 

□ 30 The source in the circuit shown in Fig. 18-20 is v t (t) = 100[u(f) - u(f - 
0.001)] V. Sketch curves as a function of <o of the amplitude of \ t (ju), H(/w) = 
V (;'w)/V i (/&)) > and V (y'w). In what way does theRC network affect the spectrum 
of the input signal? 

Fig. 18-20 See Prob. 30. 

Chapter Nineteen 

Laplace Transform Techniques 


As we begin this last chapter on the Laplace transform, it may be beneficial '*? 

to pause long enough to review our progress to date, first because we have 3 

covered a considerable amount of ground since page 1 and some tying i 

together is advisable, and secondly because we need to see how the Laplace Vf 
tmrisfiuiii liti into tuir hit-rardiv <if <iu.itytiVal method's. 

Our goal has constantly been one of analysis: given some forcing 1 

function at one point in a linear circuit, determine the response at some -,'3 

other point. For the first several chapters, we played only with dc forcing -| 

functions and responses of the form V e°. However, after the introduction Vjj 

574 Network Analysis 

of inductance and capacitance, the dc excitation of simple RL and RC 
circuits produced responses varying exponentially with time V e?'. When 
we considered the RLC circuit, the responses took on the form of the 
exponentially varying sinusoid V e at cos (bit + 0). All of this work was 
accomplished in the time domain, and the dc forcing function was the only 
one we considered. 

As we advanced to the use of the sinusoidal forcing function, the tedium 
and complexity of solving the integrodifferential equations caused us to 
begin casting about for an easier way to work problems. The phasor 
transform was the result, and we might remember that we were led to 
it through consideration of a complex forcing function of the form V e> e e>"' t . 
As soon as we concluded that we did not need the factor containing t, 
we were left with the phasor V e>"; we had arrived at the frequency domain. 

After gaming some facility in sinusoidal steady-state analysis, a modicum 
of pleasant cerebration led us to apply a forcing function of the form 
V e , 'V T+ '*' )l , and we thereby invented the complex frequency s, relegating 
all our previous functional forms to special cases: dc (s = 0), exponential 
(s = a), sinusoidal (s = ju>), and exponential sinusoid (s = a + joi). Such was 
our status at the end of Chap. 16. 

Continuing to strive for mastery over an ever greater number of differ- 
ent types of forcing functions, we turned next to nonsinusoidal periodic 
functions. Here the infinite series developed by Fourier, o + 2(a„cosruo t 
+ b n sin nu t), was found to be capable of representing almost any periodic 
function in which we might be interested. Thanks to linearity and super- 
position, the response could then be found as the sum of the responses to the 
individual sinusoidal terms. 

Remembering our success with the complex exponential function, we 
next developed the complex form of the Fourier series, 2c n e' nw <' t , suitable 
again only for periodic functions. However, by letting the period of a 
periodic sequence of pulses increase without limit, we arrived at a form 
applicable to a single pulse, the inverse Fourier transform: 

f« = -^ f *>" ( V(/<o) d» 

This then is our current status. What more could we possibly need? 
It turns out that there are several things. First, there are a few time 
functions for which a Fourier transform does not exist, such as the increasing 
exponential, many random signals, and other time functions that are not 
absolutely integrable. Second, we have not yet permitted initial-energy 
storage in the networks whose transient or complete response we desired. 
Both of these objections are overcome with the Laplace transform, and 
in addition we shall note a simpler nomenclature and ease of manipulation. 

575 tap' ** Transform Techniques 


The step that we must now take to develop the Laplace transform is 
suggested by using the inverse Fourier transform to interpret v(t) as the 
sum (integral) of an infinite number of terms, each having the form 


Upon comparing this with that of the complex forcing function, 

[V e>'V" 

which led us to the phasor V e? e , we should note that both bracketed terms 
are complex quantities in general, and, therefore, (1/2tt)V(/'£o) du> can also 
be interpreted as some kind of a phasor. Of course., the frequency differ- 
ential leads to a vanishingly small amplitude, but we add an infinite number 
of such terms together when we perform the integration. 

Our final step, therefore, parallels that which we took when we intro- 
duced phasors in the complex-frequency domain: we now let the time 
variation have the form, g ((7 +* 0>, 

To do this, let us consider the Fourier transform of e _< "«(f), rather than 
v(t) itself. Fox v(t) we have 

V(;<o) = f er*"v(t) dt (1) 



°W = a?J « MV (f»> dM 


g(t) = e-"v(t) 

we see that 

G(/<o) = J e-^'e—'vlt) dt 

= f e- ( " + '" , 'u(t) dt 


G(/<o) = V(o + ju) = J e- < » + '">'u(f) dt 



576 Na * work Analysis 

through comparison with (1). Taking the inverse Fourier transform, we 

g(f) = ijf eI " ,G(/w)d ' 

With the help of (3) we have 

e-'*v(t) =~ f e> a '\(p + iu) du 

277" J_ w 

or, upon transferring e~ at inside the integral, 

v(t) = ^f ^ +i ""V(a + fa) du 

We now replace a + /« by the single complex variable s, with ds — / dco, 
and have 

v{t) = 2^r jf° + '°° e"V(s) ds (5) 

where the limits have become a — ;'oo and a + joo. In terms of s, (4) may 
be written 

V(s) = J e-"v{t) dt (6) 

Equation (6) defines the two-sided or bilateral Laplace transform, of v(t). 
The terms "two-sided" or "bilateral" are used to emphasize the fact that 
both positive and negative times are included in the range of integration. 
Equation (5) is the inverse Laplace transform, and the two equations 
constitute the two-sided Laplace transform pair. 

If we continue the process we began earlier in this section, we may 
note that v(t) is now represented as the sum (integral) of terms of the form 



Such terms have the same form as those we encountered when we used 
phasors to represent exponentially varying sinusoids, 

[\ e> e ]e" 

5JJ Laplace Transform Techniques 

where the bracketed term was a function of s. The two-sided Laplace 
transform may therefore be interpreted as expressing v(t) as the sum 
(integral) of an infinite number of vanishingly small terms with complex 
frequency, s = a + /to. The variable is s or <o, and a should be thought 
of as governing the convergence factor e~ ot . That is, by including this 
exponential term in (6), more positive values of a ensure that the function 
e~°'v(t) u(t) is absolutely integrable for almost any v(t) that we might 
meet. The more negative values of a are needed when t < 0. Thus, the 
two-sided Laplace transform exists for a wider class of functions v(t) than 
does the Fourier transform. The exact conditions required for the ex- 
istence of the (one-sided) Laplace transform are given in the following 

In many of our circuit analysis problems, the forcing and response 
functions do not exist forever in time, but rather they are initiated at some 
specific instant that we usually select as t = 0. Thus, for time functions 
that do not exist for t < 0, or for those time functions whose behavior for 
t < is of no interest, the time-domain description can be thought of as 
v(t)u(t). The corresponding Laplace transform is then 

V(s) = f e-"v(t)u(t) dt=f e- et v(t) dt 

This defines the one-sided Laplace transform of v(t), or simply the Laplace 
transform of v(t), one-sided being understood. The inverse transform 
expression remains unchanged, but when evaluated, it is understood to be 
valid only for t > 0. Here then is the definition of the Laplace transform 
pair that will be used from now on: 

V(s) = f e-"v(t) dt 

v(t) c* V(s) 


These are memorable expressions. 

The script £ may also be used to indicate the direct or inverse Laplace 
transform operation: 


V(.) = £{v(t)} 
v(t) = £-i{V(s)} 

578 Network Analysis 

Drill Problems 

19-1 Ifo(f) = lOfor— 2<£< 1 and is zero elsewhere, determine its: (a) Fourier 
transform; (b) two-sided Laplace transform; (c) Laplace transform. 

Ans. -=^(<r 9 - 1); ^-(e- - e 2 °); -=^-(<r*" - e' 2 *>) 
s s 7« 

1 9-2 If a = 3, determine the Laplace transform of: (a) e"*'t»(*); (fo) e'u(t); (c) 
e 4 'a(f). 

Ans. i/(2 + ju); 1/(7 + ju); does not exist 

19-3 Find the Laplace transform of: (a) 2u(t); (b) e- m u{t); (c) (2 + e~ 3t )u(t). In 
each case state the range of a for which the transform exists. 

Ans. 2/s, o > 0; l/(s + 3), a > -3; (2/s) + l/(s + 3), a > 


In this section we shall begin to build up a catalog of Laplace transforms 
for those time functions most frequently encountered in circuit analysis. 
This will be done, at least initially, by utilizing the definition, 

V(s) = f e-"u(t)dt = J2{o(t)} 

which, along with the expression for the inverse transform, 

tit) = -^ f +i °° e«V(s) ds = £-'{V( S )} 
2w; J a-j x 

establishes a one-to-one correspondence between v(t) and V(s). That is, for 
every v(t) for which V(s) exists, there is a unique V(s). At this point, we 
may be looking with some trepidation at the rather ominous form given 
for the inverse transform. Fear not! As we shall see shortly, an introductory 
study of Laplace transform theory does not require actual evaluation of 
this integral. By going from the time domain to the frequency domain 
and taking advantage of the uniqueness mentioned above, we shall be able 
to generate a catalog of transform pairs such that nearly every transform 
that we wish to invert will already have the corresponding time function 
listed in our catalog. 

Before we start evaluating some transforms, however, we must pause 
to consider whether there is any chance that the transform may not even 
exist for some v(t) that concerns us. In our study of Fourier transforms, 
we were forced to take a kind of back-door approach in finding several 

579 Lap' ** Transform Techniques 

transforms. This was true with time functions that were not absolutely 
integrable, such as the unit step function. In the case of the Laplace 
transform, the use of realizable linear circuits and real-world forcing 
functions almost never leads to troublesome time functions. Technically, 
a set of conditions sufficient to ensure the absolute convergence of the 
Laplace integral for Re (s) > k are: 

1 The function v(t) is integrable in every finite interval 1 1 < t < t 2 , 
where < t t < t 2 < oo. 

2 The limit, lime _ *'|c(r)|, exists for some value of k. 


Time functions that do not satisfy these conditions are seldom encountered 
by the circuit analyst. 1 

In considering the Laplace transform of time functions having an 
impulse or higher-order singularity function at t = 0, the defining integral 
for the Laplace transform must be taken with the lower limit at t = 0~ 
in order to include the effect of the discontinuity. 2 

Now let us look at some specific transforms. In a somewhat vengeful 
mood, we first examine the Laplace transform of the unit-step function 
u(i) which caused us some earlier trouble. From the defining equation, we 
may write 

£{u(()} = f e~"u(t) dt= f e~« dt 
V s /„ s 


u(t) «• | (9) 

and our first Laplace transform pair has been established with great ease. 
Another singularity function whose transform is of considerable interest 
is the unit impulse function 8(t — t ), where t > 0": 

£{«(' - <o» = f «""" 8 (* - <o) dt = e ""° 

S(t - t ) ** e-"» (10) 

'Examples of such functions are e' ! and e" , but not t" or n'. 

2 For a further discussion on the selection of t = 0~ as the lower limit, refer to George R. 
Cooper and Clare D. McGillem, "Methods of Signal and System Analysis," Chaps. 6 and 
7, Holt, Rinehart, and Winston, New York, 1967. This text presents a somewhat more detailed 
discussion of the Laplace transform and its applications. 

580 N »tw°rk Analysis 

In particular, note that we obtain 

8(t) «* 1 (11) 

for t - 0. 

Recalling our past interest in the exponential function, we examine its 

£{e' a, u(t)} = f e- at e' at dt 

L s + a J 

S + a 

and e-"u(t) <=> —^— (12) 

s + a 

If a is negative, it is understood that Re (s) > —a. 

As a final example, for the moment, let us consider the ramp function 
tu(t). We obtain, 

£{tu(t)} = f te-"dt = \ 
J s 

tu(t) «* \ W 


either by a straightforward integration by parts or by use of a table of 
definite integrals. 

In order to accelerate the process of deriving more Laplace transform 
pairs, we shall pause to develop several useful theorems in the following 

Drill Problems 

19-4 Determine F(s) if /(f) = : (a) 5«(t); (b) 5u(t - 5); (c) 5u({ + 5). 

Ans. 5/s; 5/s; 5e- 5s /s 

19-5 Find £" 1 {V(s)} for the following V(s): (a) 2/(s + 2); (b) 2/s; (c) 2/s 2 . 

Ans. 2u(t); 2tu(t); 2e~ 2 'u(t) 

581 Laplace Transform Techniques 


The further evaluation of Laplace transforms is facilitated by applying sev- 
eral basic theorems. One of the simplest and most obvious is the linearity 
theorem: the Laplace transform of the sum of two or more time functions 
is equal to the sum of the transforms of the individual time functions. For 
two time functions we have 

JB{/iW + / 2 (*)) = f"*-'[/iW + fM dt 

= f e- t f 1 (t)dt+ f e-°%(t)dt 

= VM + F 2 (s) 

As an example of the use of this theorem, suppose that we have a Laplace 
transform V(s) and want to know the corresponding time function v(i). 
It will often be possible to decompose V(s) into the sum of two or more 
functions, say V^s) and V 2 (s), whose inverse transforms, v^t) and v 2 (t), are 
already tabulated. It then becomes a simple matter to apply the linearity 
theorem and write 

v(t) = JJ-*(V(i)} = JB-HV^i) + V 2 (s)} 

= JB-'fV^i)} + £-HV 2 ( S )} = 0l (t) + v 2 (t) 

As a specific example, let us determine the inverse Laplace transform 

V(i) = l 

(s + a)(s + /?) 

Although it is possible to substitute this expression into the defining equation 
for the inverse transform, it is much easier to utilize the linearity theorem. 
Making use of the partial fraction expansion that we all should have seen 
in our introductory calculus courses, we can split the given transform into 
the sum of two simpler transforms, 

VW ~ s + a + s + fi 

But we have already evaluated inverse transforms of the form shown on the 
right, and thus 

582 N*Nvork Analysis 

v(t) = ^-L_ e -«y f ) + _L_ e -/» aW 

If we wished we could now include this as a new entry in our catalog of 
Laplace pairs, 

^_(e-«< _ e-l»)u(t) <=> 1 — (14) 

P - a (s + o)(s + 0) K ' 

It is noteworthy that a transcendental function of t in the time domain 
transforms into a simpler rational function of s in the frequency domain. 
Simplifications of this kind are of paramount importance in transform 
theory. In this example also note that we made use of the fact that 

kv(t) <=> fcV(s) (15) 

where k is a constant of proportionality. This result is obviously a direct 
result of the definition of the Laplace transform. 

We are now able to consider two theorems that might be considered 
collectively as the raison d'etre for Laplace transforms in circuit analy- 
sis — the time differentiation and integration theorems. These will help us 
transform the derivatives and integrals appearing in the time-domain circuit 

Let us look at time differentiation first by considering a time function 
v(t) whose Laplace transform V(s) is known to exist. We want the transform 
of the first derivative of v(t), 

This can be integrated by parts, 

U=e-* dV=^dt 

with the result, 

The first term on the right must approach zero as t increases without limit; 
otherwise V(s) would not exist. Hence, 

583 Laploc« Transform Techniques 


£ (^] = - v(0) + sV(s; 

& « sV(s) - o(0) 


When there is a discontinuity at t = 0, t>(0) must be interpreted as «j(0 ). 
Similar relationships may be developed for higher-order derivatives, 

4^- <=* s 2 V(s) - st>(0) - o'(0) 

ti 3 D 

dt 3 

s 3 V(s) - s 2 u(0) - s«'(0) - c"(0) 


where e'(0) is the value of the first derivative of v(t) evaluated at * = 
(or at t - 0- if there is a discontinuity at t = 0), v"(0) is the initial value 
of the second derivative of v(t), and so forth. When all initial conditions 
are zero, we see that differentiating once with respect to t in the time 
domain corresponds to one multiplication by s in the frequency domain; 
differentiating twice in the time domain corresponds to multiplication by 
s 2 in the frequency domain, and so on. Thus, differentiation in the time 
domain is equivalent to multiplication in the frequency domain. This is 
a substantial simplification! We should also begin to see that, when the 
initial conditions are not zero, their presence is still accounted for. A simple 
example will serve to demonstrate this. 

Suppose that we have the series RL circuit shown in Fig. 19-1. The 
network is driven by a unit-step voltage, and we assume an initial value 
of the current (at t - 0~) of 5 A. 3 Using Kirchhoff 's voltage law to write 
the single loop equation in the time domain, we have 

2^- + 4i = 3u(t) 

3 We could have established this current by letting the source be 20u( 
20 — 17u(t) V, or other expressions of this nature. 

-r) + 3u(r) V, or 

Fig. 19-1 A circuit which is analyzed by transforming the differential equa- 
tion 2di/dt + 4i = 3u(r) into 2[sl(s) - 1(0-)] + 4I(s) = 3/s. 

«(«) V (+) 

•(0")-5 A 

584 Network Analysis 

Instead of solving this differential equation as we have done previously, 
we first transform to the frequency domain by taking the Laplace transform 
of each term, 

2[sI( S ) - <(0-)] + 4I( S ) = -2- 

We next solve for I(s), substituting «(0~) = 5, 



+ 4)I(s) = 

-2-+ 10 

I(s) = 


+ 5 
s + 2 

s(s + 2) 




s + 2 s 

+ 2 





s + 2 

and then use our previously determined transform pairs to invert: 

i(t) = 0.7Su(t) + 4.25e- 2t u(t) 
= (0.75 + 4.25e- 2, )u(f) 

Our solution for i(t) is complete. Both the forced response 0.75u(t) and 
the natural response 4.25e~ zt u(t) are present, and the initial condition was 
automatically incorporated into the solution. The method illustrates a very 
painless way of obtaining the complete solution of a differential equation. 
The same kind of simplification can be accomplished when we meet 
the operation of integration with respect to time in our circuit equations. 
Let us determine the Laplace transform of the time function described 
by p v(x) dx, 


£ ti' u H=.f 

e- a '\j v(x)d 

ing by parts, we let 

u = f v(x) dx 

dv = e-" dt 

du = v(f) dt 

v = -±-e- 

585 tap' ace Transform Techniques 


£ Of ** dx ) = U v{x) dx \ I - r~ 8 ']} !Io - ■£ " - 7 e ~ s,v{t) dt 

= \ _ I e -« f v(x) dx\ + - V(s) 
L s J a J o s 

But, since e" 8( -» as *-» oo, the first term on the right vanishes at the 
upper limit, and when * — » 0, the integral in this term likewise vanishes. 
This leaves only the V(s)/s term, so 


/ v(x) dx&^f- 


and thus integration in the time domain corresponds to division by s in 
the frequency domain. Once more, a relatively complicated calculus 
operation in the time domain simplifies to an algebraic operation in the 
frequency domain. 

As an example of how this helps us in circuit analysis, we shall determine 
i(t) and v(t) for t > in the series RC circuit shown in Fig. 19-2. It is 
assumed that there was some initial energy stored in the capacitor prior 
to t = so that t)(0) = 9 V. We first write the single loop equation, 

u(t) = 4i(t) + 16 J «(*) 


In order to apply the time-integration theorem, we must arrange for the 
lower limit of integration to be zero. Thus, we set 

16 T ' ilt) dt = 16 f i(t) dt + 16 f iit) dt = v(0) + 16 f i(t) dt 
J - x J -« J o "'o 


u(t) = 4i(t) + v(0) + 16 f i(i) dt 

Fig. 19-2 A circuit illustrating the use of the Laplace transform pair 

VSA " 



If F * .(f) 

c(0)-9 V 

586 Network Analysis 

We next take the Laplace transform of both sides of this equation. Since we 
are utilizing the single-ended transform, £{t>(0)} is simply £{v(0)u(t)}, and 

1 = 4I( S ) + | + JJ-I(s) 

and solving for I(s), 



s + 4 
the desired result is immediately obtained, 

i(i) = -2e- u u(t) 

If v(t) had been our desired response, we would simply have written 
a single nodal equation, 

v(t)-u(f) 1 dv 
4 16 dt 

Taking the Laplace transform, we obtain 

4 4s 16 W 16 ~ ° 



+ i) = 

s 4 


V(i) = 

4 . 


1 1 


s + 

s(s + 4) ' s 

+ 4 

s s + 4 


s s + 4 

and taking 

the inverse transform 


v(t) = 

(l + 8e 

- 4 >« 

we have quickly obtained the desired capacitor voltage without recourse 
to the usual differential equation solution. To check this result, we note 
that % 6 dv/dt should yield the previous expression for i{t). For <> 0, 

which is correct. 

To illustrate the use of both the linearity theorem and the time- 

587 Lop'*** Transform Techniques 

differentiation theorem, not to mention the addition of a most important 
pair to our forthcoming Laplace transform table, let us establish the 
Laplace transform of sin tot u(t). We could use the defining integral expres- 
sion with integration by parts, but this is needlessly difficult. Instead, we 
use the relationship, 

sin o>t = 

-L(e»"" _ e~ 


The transform of the sum of these two terms is just the sum of the trans- 
forms, and each term is an exponential function for which we already have 
the transform. We may immediately write 

£{sin atu(t)} = ^t(—^- ~ TT^ - ) = 57T" 
1 2/ vs — ;<o s + juj s' + i 

sinwtu(t) <=> 

s 2 + <o z 


We next use the time-differentiation theorem to obtain the transform of 
cos ut u(t), which is proportional to the derivative of sin u>t. That is, 

£{cosutu(«)} = £ {^tsin "*"(*)]} 

W S 2 + (O 2 


cos ut u(f) 

' + 0> 2 


Drill Problems 

1 9-6 By expansion into partial fractions, find the inverse Laplace transform of: 

(a) l/[s(s + 3)]; (b) l/^s + 3)]; (c) l/[s(s + l)(s + 3)] 

Am. V 3 (l - e- 3t )u(t); (% - %e~* + %e-*)«(t); (-% + %t + %e~ 3t )u(t) 

1 9-7 Use transform techniques to find i(t) for (> if: (a) 2 di/dt + 51 = 3a(t), 
t(0) = 4; (b) dH/df 2 + 4 di/dt + 3i = -148(f), t'(0) = 2, i(0) = 3; (c) i(«) is the 
current indicated in Fig. 19-3a. 

Ans. 5(1 + e- 2 - 5t )u(f); 1.5(3e- 3t - e-')u(t); (0.6 + 3.4e~ 2 - 5t )u(t) A 

Fig. 19-3 (a) See Drill Prob. 19-7. (b) See Drill Prob. 19-8. 





588 Artwork Analysis 

19-8 Determine v(t) for * > if: (a) 2 J"*, v(t) dt + 5v = 8; (b) 2J1„ u(t) dt + 
8 dc/dt = 8, J^ o(t) dt = 4, e(0) = 1; (c) c(f) is the indicated voltage in Fig. 19-36. 

Ans. cos (t/2)u(t); -4e-° A 'u(t); 1.6e-° A 'u{t) V 


In our study of the Fourier transform, we discovered that the Fourier 
transform of f t (t) *f 2 {t), the convolution of two time functions, was simply 
the product of the transforms of the individual functions. This then led 
to the very useful concept of the system function, defined as the ratio of 
the transform of the system output to the transform of the system input. 
Exactly the same fortunate circumstances exist when we work with the 
Laplace transform, as we shall now see. 

Let F 1 (s) and F 2 (s) be the Laplace transforms of f^t) and f 2 (t), and 
consider the Laplace transform of f^ft) * f 2 (t), 

JB{/iW •/*(*)} = £ {/ 7i(a)/»(* - \) dx) 

As we discovered in our earlier look at convolution, one of these time 
functions will often be the forcing function that is applied at the input 
terminals of a linear circuit, and the other will be the unit-impulse response 
of the circuit. That is, the response of a linear circuit is just the convolution 
of the input and the impulse response. 

Since we are now dealing with time functions that do not exist prior 
to t = (the definition of the Laplace transform forces us to assume this), 
the lower limit of integration can be changed to zero. Then, using the 
definition of the Laplace transform, we get 

£{/i« *Mt)} = fe-°» [fhWMt - A) d\] dt 

Since e -8 ' does not depend upon X, we can move this factor inside the 
inner integral. If we do this and also reverse the order of integration, the 
result is 

JB{/iM •/*«>= f [J e^'AWMt-Vd^dX 

Continuing with the same type of trickery, we note that f^X) does not 
depend upon t, so it can be moved outside the inner integral, 

£{fi(t) *Mm = f'fiW [fe-%(t - \) dt] d\ 

We then make the substitution, x = t — \, in the bracketed integral (where 
we may treat X as a constant) and, while we are at it, remove the factor 


589 Laplace Transform Techniques 

£{/iW •/.(*)} = f e_8X /i( x ) [/" e ~"f^ dx ] * 

*^0 L J 

The bracketed term is F 2 (s), which is not a function of t and can therefore 
be moved outside both integral signs. What remains is the Laplace trans- 
form F 1 (s), and we have 

/i(')*/ 2 M«Fi(s)F 2 (s) (22) 

which is the desired result. Stated slightly differently, we may conclude 
that the inverse transform of the product of two transforms is the con- 
volution of the individual inverse transforms, a result that is sometimes 
useful in obtaining inverse transforms. 

As an example of the use of the convolution theorem, let us reconsider 
the first example of Sec. 19-4, in which we were given the transform, 


(s -I- a)(s + fi) 

and obtained the inverse transform by a partial fraction expansion. We 
now identify V(s) as the product of two transforms, 

V x (») 

s + a 

™ = VTP 


o t (t) = e- at u(t) 
and v 2 (t) = erl>'u(t) 

The desired v(t) can be immediately expressed as 

v(t) = JB-HVjCsJV^s)} = v t (t) • v 2 (t) 

= f\(X)t> 2 (t-X)d\ 

= f e^V \)e-" (t - x) u(f - A) dX 

= e-f" f e l "- a)x d\ 

p — a 

590 IMwOTk Analysis 

and finally, 

v(t) = j^(e- at - e-t")u(t) 

which is the same result that we obtained before using the partial fraction 
expansion. Note that it is necessary to insert the unit step u(t) in the result 
because all Laplace transforms are valid only for nonnegative time. 

Was the result easier to obtain by this method? Not unless one is in 
love with convolution integrals. The partial-fraction-expansion method is 
usually simpler, assuming that the expansion itself is not too cumbersome. 

As we have noted several times before, the output v (t) at some point 
in a linear circuit can be obtained by convolving the input v t (t) with the 
unit-impulse response h(t). However, we must remember that the impulse 
response results from the application of a unit impulse at t = with all 
initial conditions zero. Under these conditions, the Laplace transform of 
the output is 

£RM} = v.(s) = £{»,(*) . h(t)} = \M&{HM 

Thus, the ratio V (s)/Vj(s) is equal to the transform of the impulse response, 
which we shall denote by H(s), 

£{h(t)) = H(s) = ^|| (23) 

By definition, this is known as the transfer function, the ratio of the Laplace 
transform of the output (or response) to the Laplace transform of the input 
(or forcing function) when all initial conditions are zero. The impulse 
response and the transfer function make up a Laplace transform pair. This 
is an important fact that we shall utilize later to analyze the behavior of 
some circuits that would previously have baffled us. 

Drill Problems 

19-9 Use the convolution integral to find the inverse Laplace transform of 

F^F^s) = : (a) (l/s)(l/s); (b) (l/s)(l/s) 2 ; (c) (l/s)[l/(s + 1)]. 

Ans. tu(t); (1 - <r«)u(t); ^M*) 

19-10 In the circuit of Fig. 19-4, let the input i,(t) = S(t), and determine h(t) 
and H(s) if the output is taken as: (a) v c (t); (b) i c (t); (c) i R (t). 

Ans. 50e- 5O 'u(t), S0/(s + 50); 8(t) - SOer™^), */(s + 50); 
0.5 X lO^e-^'uit), 0.5 X i0 8 /(s + 50) 


Fig. 19-4 See Drill Prob. 19-10. 


By now we have obtained a number of entries for the catalog of Laplace 
transform pairs that we agreed to construct earlier. Included are the 
transforms of the impulse function, the step function, the exponential 
function, the ramp function, the sinusoidal function, and the sum of two 
exponentials. In addition, we have noted the consequences in the s-domain 
of the time-domain operations of differentiation, integration, and convolu- 
tion; and we have used the Laplace transform to define what we mean 
by a transfer function. These results, plus several others, are collected 
together for quick reference in Tables 19-1 and 19-2. Some of the tabulated 
relationships are unfamiliar, however, and we shall now develop a few 
additional useful theorems to help us obtain them. 

As we have seen in some of our earlier transient problems, not all forcing 
functions begin at t = 0. What happens to the transform of a time function 
if that function is simply shifted in time by some known amount? In 
particular, if the transform oif(t)u(t) is the known function F(s), then what 
is the transform of f(t - a)u(t - a), the original time function delayed by 
a seconds (and not existing for t < a)? Working direcdy from the definition 
of the Laplace transform, we get 

£{/(* - a)u(t -a))= f er u f{t - a)u{t -a)dt= f" ' e—f(t - a) dt 

for t > a. Choosing a new variable of integration, t = t - a, we obtain 

£{f(t - a)u{t -a)} = f e-<~«>/(T) dr = «r"F(s) 


This result is known as the time-shift theorem, and it simply states that, 
if a time function is delayed by a time a in the time domain, the result 
in the frequency domain is a multiplication by e~ a ". 

As an example of the application of this theorem, consider the rectan- 
gular pulse described by 

v(t) = u(t - 2) - u{t - 5) 


592 N***™* Analysis 
Table 19-1 Laplace transform pairs 

fit) = £-MF(s)} 

F(s) = £{/(')} 








s 2 

— u(t), n = 1, 2, . . . 

(n - 1)1 



e "'«(*) 

s + a 



(s + af 

t- 1 


(n - 1)! 

(s + a)" 


yo — a 

(s + a)(s + /S) 


sin wt u(t) 

s 2 - + w 2 

cos u( u(<) 


s 2 + u 2 

sin (at + 9)u(t) 

s sin 9 + a cos 6 

s 2 + « 2 

cos («t + 8)u(t) 

s cos 6 — w sin 

s 2 + u 2 

e~ at sin ut u(t) 


(s + af + u 2 

e~ a% cos cof «(f) 

s + a 

(s + af + co 2 

which has unit value for the time interval, 2 < t < 5, and has zero value 
elsewhere. We know that the transform of u(t) is just 1/s, and since u(t — 2) 
is simply u(t) delayed by 2 s, the transform of this delayed function is 
e- 2e /s. Similarly, the transform of u(t — 5) is e~ 5e /s. It follows, then, that 
the desired transform is 

V(s) = ■ 

It was not necessary to revert to the definition of the Laplace transform 
in order to determine V(s). 

The time-shift theorem is also useful in evaluating the transform of 

593 toplace Transform Techniques 

periodic time functions. Suppose that f(t) is periodic with a period T for 
positive values of t. The behavior of f(t) f or t < has no effect on the 
(one-sided) Laplace transform, as we know. Thus, f(t) can be written as 

/(f) = f(t -nT) n = 0, 1, 2, . . . 

If we now define a new time function which is nonzero only in the first 
period of f(t), 

/,(() = [u(t) - u(t - T)]f(t) 

Table 19-2 Laplace transform operations 






F,(») ± F 2 (») 





Time differen- 


sF(s) - /(0) 

dt 2 

s 2 F( s ) - s/(0) - f(0) 

d 3 f 


s 3 ^) - S J(0) _ sf (0) - /"(0) 

Time integration 

f f(t)dt 


f f(t) dt 

7 F(s) + i/° /Wd ' 



F,(»)F 2 (s) 

Time shift 

f(t - a)u(t - 

- a), a > 


Frequency shift 


F(s + a) 

Frequency dif- 



Frequency inte- 


j F(s)ds 


f(at), a > 


Initial value 


Iim sF(s) 

8— >00 

Final value 


lim sF(s), all poles of sF(s) in LHP 


Time periodicity 

/»=/(* + 

nT), n = 1, 2, . . . 

1 _ e -T.*M "*ere F^s) - j f(t) e •< dt 

594 Network Analysis 

then the original f(t) can be represented as the sum of an infinite number 
of such functions, delayed by integral multiples of T. That is, 

f(t) = [u(t) - u(t - T)]f(t) + [u(t - T) - u(t - 2T)]f(t) 

+ [u(t - 2T) - u(t - 3T)]f(t) + ■■■ 

= /i(*)+/i(*-r)+/ 1 (t-2T)+ ••• 
or /(*) = 2 hit - nT) 


The Laplace transform of this sum is just the sum of the transforms, 

f(s) = 2 £ {/i(* - nT )J 


so that the time-shift theorem leads to 

F(s) = J s-TiW 


F 4 (s) - £{/ t (*)} = f T e-*f(t)dt 

Since F 1 (s) is not a function of n, it can be removed from the summation, 
and F(s) becomes 

F(s) = F 1 (s)[l + e- Ts + e~ 2T * + • • •] 

When we apply the binomial theorem to the bracketed expression, it 
simplifies to 1/(1 — e' Ta ). Thus, we conclude that the periodic function 
/(*), with period T, has a Laplace transform expressed by 

F ( s ) = rrF- (25) 


F^s) = £{[u(t) - u(t - T)]f(t)} (26) 

is the transform of the first period of the time function. 

To illustrate the use of this transform theorem for periodic functions, 
let us apply it to the familiar rectangular pulse train, Fig. 19-5. We may 
describe this periodic function analytically: 

v(t) = 2 V [u(t - nT) - u(t -nT-r)] t>0 


T T+T 

2T ar+r 

Fig. 19-5 A periodic train of rectangular pulses for which F(s) = 
(V /s|(l - e-')/(l - e" T ). 

The function V^s) is simple to calculate, 

Vj(s) = V f T e-"dt = ^2(1 - tr") 

Now, to obtain the desired transform, we just divide by (1 — e~ 87 ), 

v ( .) = ^ - 1 - e ~ 

s 1 — e~ 


We should note how the two theorems described in this section show up 
in the transform (27). The (1 — e~ aT ) factor in the denominator accounts 
for the periodicity of the function, the e~" T term in the numerator arises 
from the time delay of the negative square wave that turns off the pulse, 
and the V /s factor is, of course, the transform of the step functions involved 
in v(t). 

Drill Problems 

19-11 Determine the Laplace transform of the functions of time depicted in 
Fig. 19-6. 

Am. 1.5(1 - e~ 2s )/s 2 ; 1.5e-*(l - e' 2a )/s 2 ; 1.5{e~ s - e~ 3 *)(l - e~ 2 °)/s 2 

Fig. 19-6 See Drill Prob. 1 9-1 1 . 








5 <( S ) 


596 Network Analysis 

19-12 Find the Laplace transforms of the periodic functions illustrated in Fig. 

Ans. 10/(1 - e-* /5 ); (50/s 2 ) - i0e-°- 2s /(s - se" - 2 "); 
(10/s)(e-' no - e- /s )/(l - e-°- 3s ) 



[10) (10) 



0.2 0.4 0.6 < (s) 
Fig. 19-7 See Drill Prob. 19-12. 

0.2 0.4 0.6 t (s) 

0.2 0.4 0.6 t (s) 


Other theorems appearing in Table 19-2 specify the results in the time 
domain of simple operations on s in the frequency domain. We shall obtain 
several easily in this section and then see how they may be applied to derive 
additional transform pairs. 

The first new theorem establishes a relationship between F(s) = £{/(*)} 
and F(s + a). We consider the Laplace transform of e~ at f(t), 

£{e—f(t))= f e-«e-° t f(t)dt= C~e-< M *f(t)dt 

J o o 

Looking carefully at this result, we note that the integral on the right is 
identical to that defining F(s) with one exception: (s + a) appears in place 
of s. Thus, 

e-"'f(t) <=> F(s + a) 


Thus, we conclude that replacing s by (s + a) in the frequency domain 
corresponds to multiplication by e' at in the time domain. This is known 
as the frequency-shift theorem. It can be put to immediate use in evalu- 
ating die transform of the exponentially damped cosine function that we 
used extensively in previous work. Beginning with the known transform 
of the cosine function, 

£{cos<o t} = F(s) 

S" + u 

397 Laplace Transform Techniques 

then the transform of e~ ttt cos u t must be F(s 4- a), 

£{<r°< c -° s »<>*> = F(« + «) = (S+ ( ^; ) V (29) 

Next let us examine the consequences of differentiating F(s) with respect 
to s. The result is 

n^ = sl e -" fit)dt 

= f -te-"f(t)dt 
= f e-"[-tf(t)]dt 

which is clearly the Laplace transform of [—tf(t)]. We therefore conclude 
that differentiation with respect to s in the frequency domain results in 
multiplication by — t in the time domain, or 

-tf(t) ** ^F(s) (30) 

Suppose now that f(t) is the unit-ramp function tu(t) whose transform 
we know is l/s z . We can use our newly acquired frequency-differentiation 
theorem to determine the inverse transform of 1/s 3 as follows: 


Continuing with the same procedure, we find 

3T"M ~ } (32) 

and in general 

598 Nelwor ' ( Anolysi* 

The effect on f(t) of integrating F(s) with respect to s may be shown 
by beginning with the definition once more, 

F(s) = f e~"f(t) dt 

performing the frequency integration from s to oo, 

f F(s) ds = f \j er"f(t) dt\ ds 

interchanging the order of integration, 

J"°°F(s)ds = J [J* e-" ds]/(t) dt 

and performing the inner integration, 


M<=> f°F(s) ds (34) 

For example, we have already established the transform pair, 

sin u t u(i) 

«2 J. ,.,2 

s* + «„* 


fsin^oilfW] = f "o* = tan -! J_ I " 
I t J J 9 s 2 + « 2 " I S 

and we have 

sin<yu(t) Q ^_ tan -tJ_ (35) 

f 2 w 

We next develop the time-scaling theorem of Laplace transform theory 
by evaluating the transform of fiat), assuming that £ {fit)} is known. The 
procedure is very simple: 

£{f(at))= f™e-°*fiat)dt = ~( ^-"^/(A) dX 

599 Laplace Transform Techniques 

where the change of variable, at = A, has been employed. The last integral 
is recognizable as 1/a times the Laplace transform of /(£), except that s 
is replaced by s/a in the transform. It follows that 

f(at) <=> -F(s/a) (36) 

As an elementary example of the use of this time-scaling theorem, consider 
the determination of the transform of a 1-kHz cosine wave. Assuming we 
know the transform of a 1-rad/s cosine wave, 

cos t u(t) 

s 2 + 1 

the result is 

1 s/20(Xk- 

£{cos20007rfu(t)} = 

2000tt (s/2000w) 2 + 1 s 2 + (2000u) 2 

which is correct. 

The time-scaling theorem offers us some computational advantages, for 
it enables us to work initially in a slowed-down world, where time functions 
may extend for several seconds and periodic functions possess periods of 
the order of magnitude of a second. Practical engineering work, however, 
usually involves time functions that vary much more rapidly with time than 
our examples might have indicated. The time slowdown is used only to 
simplify the computational aspects of our problems. These results may then 
be translated easily to the real world through the use of the time-scaling 

Drill Problems 

19-13 Find: (a) £r l {Va/[(s + 3) 2 + 4]}; (b) £r l { e - 3 - 3 /(s + 1)}; (c) £" 1 {2/ 
[(» + 3) 2 ]}. 

Ans. e~'u(t - 3); 2e'- 3 'tu(t)i 5e~ 3 ' sin2tu(t) 

19-14 Find the Laplace transform of: (a) te- 2t u(t); (b) t 2 er 2t u(t); (c) t 3 e- 2 'u(t). 

Ans. l/(s + 2f ; 2/(s -I- 2f ; 6/(s + 2f 

19-15 If £-i{s~ 5/2 } = (4*3/2/3 VS)u(t). find: .(a) S-^s^ 2 }; (b) i-ifs" 1 / 2 }- 
(c) £-i{s- 7 / 2 }. 

Ans. {r 1/2 /\fr)u(t) ; (2t 1/2 /\fH)u(t); (8fi /2 /15\^)u(t) 

19-1* If £{/(*)} = (s 2 -(- l)/(s? + s 2 + 1), determine the Laplace transform of: 

(a) f(2t); (b) f(t/2); (c) tf(t). 

Ans 1 tjJt j ** + 4 3 «V + %) 

' 4 s 5 + s 2 /S + y 32 ' s 5 + 8s 2 + 32 ' (s 5 + s 2 + If 

600 Network Analysis 


The last two fundamental theorems that we shall discuss are known as the 
initial-value and final- value theorems. They will enable us to evaluate /(0 + ) 
and /(oo) by examining the limiting values of F(s). 

To derive the initial-value theorem, we consider the Laplace transform 
of the derivative once again, 

£ {|}= S F( S )-/(0-)=^ e -|* 

We now let s approach infinity. By breaking the integral into two parts, 

lim [«F(i) -/(0-)] = lira (f° e°fdt + f e-'^-dt) 

we see that the second integral must approach zero in the limit since the 
integrand itself approaches zero. Also, /(0~) is not a function of s, and 
it may be removed from the left limit, 

-/(0-) + lim [sF(s)] = lim f ° df = lim [/(0+) - /(0")] 

= /(o + ) - /(0-) 

and finally 

/(0+) = lim [sF(s)] 

or lim/(f)= lim[sF(s)] (37) 

This is the mathematical statement of the initial-value theorem. It states 
that the initial value of the time function f(t) can be obtained from its 
Laplace transform F(s) by first multiplying the transform by s and then 
letting s approach infinity. Note that the initial value of /(f) that is obtained 
is the limit from the right. 

The initial-value theorem, along with the final-value theorem that we 
shall consider in a moment, is useful in checking the results of a trans- 
formation or an inverse transformation. For example, when we first calcu- 
lated the transform of cos ic t u(t), we obtained s/(s 2 + w 2 ). After noting 
that/(0 + ) = 1, a partial check on the validity of this result is achieved by 
applying the initial-value theorem, 

8^,0 \ S 2 + « 2 / 

and the check is accomplished. 

60 1 Laplace Transform Technique* 

The final-value theorem is not quite as useful as the initial-value theo- 
rem, for it can be used only with a certain class of transforms, those whose 
poles lie entirely within the left half of the s plane, except for a simple 
pole at s = 0. We again consider the Laplace transform of df/dt, 

fe-'^dt = sF( S )-f(0-) 

this time in the limit as s approaches zero, 

lira f er"^.dt= lim [sF(s) - f(Q-)] = f % 
•-o J - dt s-^o J J - dt 


We assume that both f(t) and its first derivative are transformable. Now, 
the last term of this equation is readily expressed as a limit, 

By recognizing that /(0~) is a constant, a comparison of the last two equa- 
tions shows us that 

lim f{t) = lim [sF(s)] (38) 

t-»oo s— >0 

which is the final-value theorem. In applying this theorem, it is necessary 
to know that /(oo), the limit of f(t) as t becomes infinite, exists, or, what 
amounts to the same thing, that the poles of sF(s) all lie within the left 
half of the s plane; they may not even lie on the ;'co axis. 

As a straightforward example of the application of this theorem, let 
us consider the function /(t) = (1 — e~ at )u(f), where a > 0. We see imme- 
diately that/(oo) = 1. The transform of /(f) is 

F(i) = I - 


s s + a s(s + a) 
Multiplying by s and letting s approach zero, we obtain 

lim [sF(s)l = lim — ^— = 1 
»-*o s-^o s + a 

which agrees with /(oo). 

If f(t) is a sinusoid, however, so that F(s) has poles on the ;'co axis, then 
a blind use of the final-value theorem might lead us to conclude that the 
final value is zero. We know, however, that the final value of either sin oi t 
or cos u t is indeterminate. So, beware of /co-axis poles. 

602 N » lw ««* Analysis 

We now have all the tools to apply the Laplace transform to the solution 
of problems that we either could not solve previously, or that we solved 
with considerable stress and strain. 

Drill Problem 

19-17 Find/(0 + ) and/(oo) for each of the following transforms, without deter- 
mining/^) first: (a) (2 - e" 38 )/[s(s 2 + s + 4)]; (b) 2s/(s 2 + s + 4); (c) 2/(1 - e—). 

Ans. 0, 0.25; 2, 0; oo, unknown 


Earlier in this chapter we defined the transfer function H(s) as the Laplace 
transform of the impulse response h(t), initial energy being zero throughout 
the circuit. Before we can make the most effective use of the transfer 
function, we need to show that it may be obtained very simply for any 
linear circuit by frequency-domain analysis. We do this by an argument 
similar to that presented for the Fourier transform and H(/w) in Sec. 18-9. 
But we shall be brief. 

We work in the complex-frequency domain and apply an input, v t (t) = 
Ae" xt cos (o> x t + 0), which is V 4 (s # ) = Ae' e in phasor form. Both A and 
are functions of s x — a x + j<c x , the complex frequency of the excitation. 
The response is v (i) = Be"-* cos (u„t + </>), V„(sJ = Be"*. Thus, 

^ = G( Sl ) = !**"> (39) 

To determine H(s), we need to find the ratio of the transform of the output 
to the transform of the input, 

£{Be°'> cos (uj + <t>)} 
U £{Ae*"' cos(u x t + 0)} 

The required transform is obtained from Table 19-1 by replacing s by s — a x 
in the transform for cos (at + 0). We have 

f [(s - a x ) cos <j> - u, sin <j>] ] 
I [(• - o x f + CO/] j 

H( S) - - [ (S - ^ + "* 2] 

A \ [( S ~ ^ C0S 9 ~ "« Si " ^i I 

A \ [(. - a x f + u *\ J 

603 Laplace Transform Techniques 

At s = s x , this simplifies to 

B ju„ cos <j> — <Jg sin <ft 
(Sl)_ A /u,cosfl -u,sine 

_ B cos<j> + ;sin<fr _ _B gi(0 _ 9) 
A cos 5 + ;'sin0 A 

which is identical to (39). Since there is no special significance to the x 
subscript, it follows that 

H(s) = G(s) 


Thus, we may find H(s) by using normal frequency-domain methods with 
all elements expressed in terms of their impedances at a complex fre- 
quency s. 

Let us illustrate how this technique may be used to find both h(t) and 
an output voltage for the circuit shown in Fig. 19-8a. At this time we 
assume that there is no initial energy storage in the network. We first 
construct the frequency-domain circuit, shown in Fig. 19-8i». The ratio 
of V (s)/ V 4 (s) may be found by determining Z,(s), the impedance of the three 
parallel branches at the right, 

Z,(s) = 

1 120(s + 2) 

s/24 + y 30 + 1/(24 + 48/s) ~~ 5s 2 + 19s + 8 

Fig. 19-8 (a) An example in which the transfer function H(s) = V^sl/Vjls) 
is to be obtained by frequency-domain analysis. Initial conditions are all zero. 
[b] The frequency-domain circuit. 

=T= "oO 

20 a , 



24 a; 

30 a'. 

\ ^= 



604 Network Analysis 

and then using voltage division, 

v .w = z j( s ) -_ 6 ( s + 2 ) 

V;(s) 20 + Z,(s) 5s 2 + 25s + 20 

WA = 1 - 2 ( s + 2 ) 
u (s + l)(s + 4) 

To find fc(f), we need £- x {H(s)}: 

^ £BW) = ^{ i M r+ -M_} 

and fc(t) = (0.4e"' + 0.8e"")u(t) 

Thus, if e,(r) = S(t), o (t) = h(t) = (0.4e- ( + 0.8<T 4 >(t). 

For a different input, say v t (t) = 50 cos 2t u(t) V, we may make use of 
the transfer function concept, 

v„(i) = mm*) 


V,(s) = £{50 cos 2tu(t)} = - g 50 * 

and V (s) = 

s 2 + 4 
1.2(s + 2) 50s 

(s + l)(s + 4) s 2 + 4 

Expanding in partial fractions, 

.... -4 -8 6 + « 6- 

v »( s ) = T-r^r + ^rm + ^4r + 

s+l s + 4 s + /2s-/2 

_ -4 . -8 , 12s + 24 
s+l s + 4 s 2 + 4 

and »„(() = (-4e" ( - 8e-« + 12 cos 2f + 12 sin 2f)u(f) 

The solution is straightforward, and we should feel confident of being 
able to find the response for any input that is Laplace-transformable. We 
consider the presence of initial-energy storage in the next (and final) section. 

Drill Problem 

19-18 Find the impulse response of the circuit of Fig. 19-9 by constructing the 
frequency-domain circuit, finding the appropriate transfer function, and evaluating 
the inverse Laplace transform. The output is: (a) v A (t); (b) u B (t); (c) v c (t). 

Ans.(6e- 4 ' - 24te- 4t )u(t); 8(f) - (6e- 4 > - 8UT 4 ')u(ty, (6e-« - 8f<r 4 >(f) 




+ ° c(0 " ±+ ±+ 

":(>)(-) 2Q<" A (0 6a<f B (<) 

Fig. 19-9 See Drill Prob. 19-18. 


When initial energy is present in a circuit, the Laplace transform method 
may be used to obtain the complete response by any of several different 
methods. We shall consider two of them. 

The first is the more fundamental, for it involves writing the differential 
equations for the network and then taking the Laplace transform of those 
equations. The initial conditions appear when a derivative or integral is 
transformed. The second technique requires each initial capacitor voltage 
or inductor current to be replaced by an equivalent dc source, often called 
an initial-condition generator. The elements then carry no initial energy, 
and the transfer function procedure of the preceding section can be fol- 

Let us illustrate the differential equation approach by considering the 
same circuit we just analyzed, but with nonzero initial conditions this time, 
as shown in Fig. 19-10. We let c^O") = 10 V and « 2 (0-) - 25 V. 

The differential equations for this circuit may be obtained by writing 
nodal equations in terms of v x and t> 2 . At the t> x node, 

+ 48°i=° 


2v 2 — 2«j + v[ 


Fig. 19-10 The response v 2 {t) is obtained for this network with the initial 
conditions, 1^(0") = 10 V, v 2 [Q-) = 25 V. 

l 2t «(*) (+) 


+ -^ + -^rv' ? = 

506 N **w°rk Analysis 

while at the v 2 node, 

v 2 — 50 cos 2t u(t) 

20 """ 24 " r 30" r 24" 2 

or *>! = c> 2 + 3u 2 - 60 cos 2f u(t) (42) 

Identifying v 2 as the desired response, we eliminate v x and «i by taking 
the derivative of (42), remembering that du(t)/dt = 8(t), 

v[ = v 2 + 3v' 2 + 120 sin %t u(t) - 60«(f) (43) 

and substituting (42) and (43) into (41), 

2u 2 = 2[t> 2 + 3c 2 - 60cos2fu(f)] + [v' 2 ' + 3v' 2 + 120sin2f«(f) - 608(f)] 
or t>2 + 5v' 2 + 4v 2 = (120 cos 2f - 120 sin 2t)u(i) + 605(f) 

We now take the Laplace transform, 

s 2 V 2 (s) - w^O-) - v' 2 (0-) + 5sV 2 (s) - 5« 2 (0-) + 4V 2 (s) = ^ ~ 240 + 60 

collect terms, 

( S 2 + 5s + 4)V 2 (s) = St , 2 (0") + v' 2 (0-) + 5» 2 (0-) + 120s -240 + ^ 

let u 2 (0-) = 25, 

( S 2 + 5s + 4)V 2 (s) = 25s + 125 + v' 2 (0~) + 120 2 ~ 240 + 60 

S +4 

and need a value for t>2(0~). This we mav obtain from the two circuit 
equations (41) and (42) by evaluating each term at t = 0~. Actually, we 
need use only (42) in this problem: 

Cl (0-) = o 2 (0") + 3» 2 (0-) - 
and t> 2 (0") = -65 


,. , . 25s + 120 + 120[(s - 2)/(s 2 + 4)] 

(s + l)(s + 4) 

25s 3 + 120s 2 + 220s + 240 

~ (s + l)(s + 4)(s 2 + 4) 

2 % »% 12s + 24 

s + ls + 4 s 2 + 4 











Li(0-)( + ) V(s) 





Fig. 19-1 1 (o) An inductor L with initial current i[0~) is shown in the time 
domain, (b) and (c) Frequency-domain networks that are equivalent to (a) 
for Laplace-transform analysis. 

from which the time-domain response is obtained, 

v 2 (t) = ( 2 %e-' + 16 / 3 e- 4 » + 12 cos 2t + 12 sin 2*)u(t) 

Now let us determine the frequency-domain equivalent of an inductor 
L with initial current i(0~). The time-domain network of Fig. 19-1 la is 
described by 

v(t) = Li' 

and, therefore, 

V(s) = sLl(s) - Lt(0-) 


The frequency-domain equivalents can be read directly from (45) and (46), 
and they are shown in Figs. 19-1 lb and c, respectively. It may be helpful 
to note that the voltage source in Fig. 19-1 lfo is the transform of an impulse, 
while the current source in c is the transform of a step. 

Equivalent networks for an initially charged capacitor are obtained by 
a similar procedure; the results are shown in Fig. 19-12. 

Fig. 19-12 (a) A capacitor C with initial voltage v{0~) is shown in the time 
domain, {b) and (c) Frequency-domain networks that are equivalent to (a) 
for Laplace-transform analysis. 







Jz (t) c«,(o-) 

Fig. 19-13 The frequency-domain equivalent of the circuit of Fig. 19-10. 
The current sources 10 / iS and 2 % 4 provide initial time-domain voltages of 10 
and 25 V across the %8-F and %4-F capacitors, respectively. 

We may now use these results to construct a frequency-domain equiva- 
lent of the circuit shown in Fig. 19-10, including the effect of the initial 
conditions. The result is shown in Fig. 19-13. Current sources are used 
for the initial conditions to expedite the writing of nodal equations. 

We must now use both the superposition principle and the concept of 
the transfer function to see that V 2 (s) is composed of the sum of three terms, 
one due to each source acting alone. Moreover, each of these sources has 
a transfer function to V 2 (s). Each transfer function could be obtained by 
applying the standard frequency-domain analysis methods. We need not 
solve three little problems, however, for we can accomplish the fre- 
quency-domain analysis with all three sources operating. We do t